Radial Velocity Dispersions of Star Groups in M67
High-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical spa...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Vereshchagin S. V. [verfasserIn] Chupina N. V. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
In: Open Astronomy - De Gruyter, 2018, 25(2016), 4, Seite 432-438 |
|---|---|
| Übergeordnetes Werk: |
volume:25 ; year:2016 ; number:4 ; pages:432-438 |
| Links: |
|---|
| DOI / URN: |
10.1515/astro-2017-0263 |
|---|
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DOAJ059987251 |
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| 520 | |a High-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical space velocities was confirmed. The possibility of more accurate future studies of the parameters of star groups using the Gaia catalogues is discussed. | ||
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10.1515/astro-2017-0263 doi (DE-627)DOAJ059987251 (DE-599)DOAJ2411a6c467454bf9898dc67c2b6cc9db DE-627 ger DE-627 rakwb eng QB1-991 Vereshchagin S. V. verfasserin aut Radial Velocity Dispersions of Star Groups in M67 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier High-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical space velocities was confirmed. The possibility of more accurate future studies of the parameters of star groups using the Gaia catalogues is discussed. solar neighborhood open clusters and associations: individual (m 67) Astronomy Chupina N. V. verfasserin aut In Open Astronomy De Gruyter, 2018 25(2016), 4, Seite 432-438 (DE-627)1000905144 (DE-600)2908865-3 25436376 nnns volume:25 year:2016 number:4 pages:432-438 https://doi.org/10.1515/astro-2017-0263 kostenfrei https://doaj.org/article/2411a6c467454bf9898dc67c2b6cc9db kostenfrei https://doi.org/10.1515/astro-2017-0263 kostenfrei https://doaj.org/toc/2543-6376 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ AR 25 2016 4 432-438 |
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High-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical space velocities was confirmed. The possibility of more accurate future studies of the parameters of star groups using the Gaia catalogues is discussed. |
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High-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical space velocities was confirmed. The possibility of more accurate future studies of the parameters of star groups using the Gaia catalogues is discussed. |
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High-precision measurements of radial velocities of the M67 cluster members are used to calculate the radial-velocity dispersions in the stellar groups found earlier in the cluster’s corona. The previously detected feature in one of the groups (Group 60) consisting of stars with almost identical space velocities was confirmed. The possibility of more accurate future studies of the parameters of star groups using the Gaia catalogues is discussed. |
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