Masers: Precision probes of molecular gas
Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Richards, A.M.S. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2020transfer abstract |
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| Schlagwörter: |
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| Umfang: |
10 |
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| Übergeordnetes Werk: |
Enthalten in: Posttranscriptional actions of triiodothyronine on - Bargi-Souza, Paula ELSEVIER, 2018, including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU), Amsterdam [u.a.] |
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| Übergeordnetes Werk: |
volume:65 ; year:2020 ; number:2 ; day:15 ; month:01 ; pages:780-789 ; extent:10 |
| Links: |
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| DOI / URN: |
10.1016/j.asr.2019.05.052 |
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ELV048976121 |
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| 520 | |a Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. | ||
| 520 | |a Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. | ||
| 650 | 7 | |a Stars: mass loss |2 Elsevier | |
| 650 | 7 | |a Star formation |2 Elsevier | |
| 650 | 7 | |a Planetary systems: protoplanetary disks |2 Elsevier | |
| 650 | 7 | |a Masers |2 Elsevier | |
| 650 | 7 | |a Stars: supergiant |2 Elsevier | |
| 650 | 7 | |a Stars: AGB |2 Elsevier | |
| 700 | 1 | |a Sobolev, A. |4 oth | |
| 700 | 1 | |a Baudry, A. |4 oth | |
| 700 | 1 | |a Herpin, F. |4 oth | |
| 700 | 1 | |a Decin, L. |4 oth | |
| 700 | 1 | |a Gray, M.D. |4 oth | |
| 700 | 1 | |a Etoka, S. |4 oth | |
| 700 | 1 | |a Humphreys, E.M.L. |4 oth | |
| 700 | 1 | |a Vlemmings, W. |4 oth | |
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10.1016/j.asr.2019.05.052 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000862.pica (DE-627)ELV048976121 (ELSEVIER)S0273-1177(19)30421-1 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Richards, A.M.S. verfasserin aut Masers: Precision probes of molecular gas 2020transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Stars: mass loss Elsevier Star formation Elsevier Planetary systems: protoplanetary disks Elsevier Masers Elsevier Stars: supergiant Elsevier Stars: AGB Elsevier Sobolev, A. oth Baudry, A. oth Herpin, F. oth Decin, L. oth Gray, M.D. oth Etoka, S. oth Humphreys, E.M.L. oth Vlemmings, W. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:2 day:15 month:01 pages:780-789 extent:10 https://doi.org/10.1016/j.asr.2019.05.052 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 2 15 0115 780-789 10 |
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10.1016/j.asr.2019.05.052 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000862.pica (DE-627)ELV048976121 (ELSEVIER)S0273-1177(19)30421-1 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Richards, A.M.S. verfasserin aut Masers: Precision probes of molecular gas 2020transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Stars: mass loss Elsevier Star formation Elsevier Planetary systems: protoplanetary disks Elsevier Masers Elsevier Stars: supergiant Elsevier Stars: AGB Elsevier Sobolev, A. oth Baudry, A. oth Herpin, F. oth Decin, L. oth Gray, M.D. oth Etoka, S. oth Humphreys, E.M.L. oth Vlemmings, W. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:2 day:15 month:01 pages:780-789 extent:10 https://doi.org/10.1016/j.asr.2019.05.052 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 2 15 0115 780-789 10 |
| allfields_unstemmed |
10.1016/j.asr.2019.05.052 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000862.pica (DE-627)ELV048976121 (ELSEVIER)S0273-1177(19)30421-1 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Richards, A.M.S. verfasserin aut Masers: Precision probes of molecular gas 2020transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Stars: mass loss Elsevier Star formation Elsevier Planetary systems: protoplanetary disks Elsevier Masers Elsevier Stars: supergiant Elsevier Stars: AGB Elsevier Sobolev, A. oth Baudry, A. oth Herpin, F. oth Decin, L. oth Gray, M.D. oth Etoka, S. oth Humphreys, E.M.L. oth Vlemmings, W. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:2 day:15 month:01 pages:780-789 extent:10 https://doi.org/10.1016/j.asr.2019.05.052 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 2 15 0115 780-789 10 |
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10.1016/j.asr.2019.05.052 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000862.pica (DE-627)ELV048976121 (ELSEVIER)S0273-1177(19)30421-1 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Richards, A.M.S. verfasserin aut Masers: Precision probes of molecular gas 2020transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Stars: mass loss Elsevier Star formation Elsevier Planetary systems: protoplanetary disks Elsevier Masers Elsevier Stars: supergiant Elsevier Stars: AGB Elsevier Sobolev, A. oth Baudry, A. oth Herpin, F. oth Decin, L. oth Gray, M.D. oth Etoka, S. oth Humphreys, E.M.L. oth Vlemmings, W. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:2 day:15 month:01 pages:780-789 extent:10 https://doi.org/10.1016/j.asr.2019.05.052 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 2 15 0115 780-789 10 |
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10.1016/j.asr.2019.05.052 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000000862.pica (DE-627)ELV048976121 (ELSEVIER)S0273-1177(19)30421-1 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Richards, A.M.S. verfasserin aut Masers: Precision probes of molecular gas 2020transfer abstract 10 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. Stars: mass loss Elsevier Star formation Elsevier Planetary systems: protoplanetary disks Elsevier Masers Elsevier Stars: supergiant Elsevier Stars: AGB Elsevier Sobolev, A. oth Baudry, A. oth Herpin, F. oth Decin, L. oth Gray, M.D. oth Etoka, S. oth Humphreys, E.M.L. oth Vlemmings, W. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:65 year:2020 number:2 day:15 month:01 pages:780-789 extent:10 https://doi.org/10.1016/j.asr.2019.05.052 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 65 2020 2 15 0115 780-789 10 |
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Enthalten in Posttranscriptional actions of triiodothyronine on Amsterdam [u.a.] volume:65 year:2020 number:2 day:15 month:01 pages:780-789 extent:10 |
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Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. |
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Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. |
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Maser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures ≫ 10 10 K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales ≪ 1 mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases. |
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Sobolev, A. Baudry, A. Herpin, F. Decin, L. Gray, M.D. Etoka, S. Humphreys, E.M.L. Vlemmings, W. |
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