A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars

Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbioti...
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Gespeichert in:

Autor*in:	Paula Esther Marchiano [verfasserIn] María Laura Arias [verfasserIn] Michaela Kraus [verfasserIn] Michalis Kourniotis [verfasserIn] Andrea Fabiana Torres [verfasserIn] Lydia Sonia Cidale [verfasserIn] Marcelo Borges Fernandes [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Schlagwörter:	techniques: spectroscopic stars: symbiotic, binaries stars: infrared

Übergeordnetes Werk:	In: Galaxies - MDPI AG, 2013, 11(2023), 4, p 80
Übergeordnetes Werk:	volume:11 ; year:2023 ; number:4, p 80

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/galaxies11040080

Katalog-ID:	DOAJ093614438

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allfields	10.3390/galaxies11040080 doi (DE-627)DOAJ093614438 (DE-599)DOAJ38d0e648f00e47ad83183065fc2b836a DE-627 ger DE-627 rakwb eng QB1-991 Paula Esther Marchiano verfasserin aut A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems. techniques: spectroscopic stars: symbiotic, binaries stars: infrared Astronomy María Laura Arias verfasserin aut Michaela Kraus verfasserin aut Michalis Kourniotis verfasserin aut Andrea Fabiana Torres verfasserin aut Lydia Sonia Cidale verfasserin aut Marcelo Borges Fernandes verfasserin aut In Galaxies MDPI AG, 2013 11(2023), 4, p 80 (DE-627)730276740 (DE-600)2691049-4 20754434 nnns volume:11 year:2023 number:4, p 80 https://doi.org/10.3390/galaxies11040080 kostenfrei https://doaj.org/article/38d0e648f00e47ad83183065fc2b836a kostenfrei https://www.mdpi.com/2075-4434/11/4/80 kostenfrei https://doaj.org/toc/2075-4434 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 11 2023 4, p 80
spelling	10.3390/galaxies11040080 doi (DE-627)DOAJ093614438 (DE-599)DOAJ38d0e648f00e47ad83183065fc2b836a DE-627 ger DE-627 rakwb eng QB1-991 Paula Esther Marchiano verfasserin aut A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems. techniques: spectroscopic stars: symbiotic, binaries stars: infrared Astronomy María Laura Arias verfasserin aut Michaela Kraus verfasserin aut Michalis Kourniotis verfasserin aut Andrea Fabiana Torres verfasserin aut Lydia Sonia Cidale verfasserin aut Marcelo Borges Fernandes verfasserin aut In Galaxies MDPI AG, 2013 11(2023), 4, p 80 (DE-627)730276740 (DE-600)2691049-4 20754434 nnns volume:11 year:2023 number:4, p 80 https://doi.org/10.3390/galaxies11040080 kostenfrei https://doaj.org/article/38d0e648f00e47ad83183065fc2b836a kostenfrei https://www.mdpi.com/2075-4434/11/4/80 kostenfrei https://doaj.org/toc/2075-4434 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 11 2023 4, p 80
allfields_unstemmed	10.3390/galaxies11040080 doi (DE-627)DOAJ093614438 (DE-599)DOAJ38d0e648f00e47ad83183065fc2b836a DE-627 ger DE-627 rakwb eng QB1-991 Paula Esther Marchiano verfasserin aut A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems. techniques: spectroscopic stars: symbiotic, binaries stars: infrared Astronomy María Laura Arias verfasserin aut Michaela Kraus verfasserin aut Michalis Kourniotis verfasserin aut Andrea Fabiana Torres verfasserin aut Lydia Sonia Cidale verfasserin aut Marcelo Borges Fernandes verfasserin aut In Galaxies MDPI AG, 2013 11(2023), 4, p 80 (DE-627)730276740 (DE-600)2691049-4 20754434 nnns volume:11 year:2023 number:4, p 80 https://doi.org/10.3390/galaxies11040080 kostenfrei https://doaj.org/article/38d0e648f00e47ad83183065fc2b836a kostenfrei https://www.mdpi.com/2075-4434/11/4/80 kostenfrei https://doaj.org/toc/2075-4434 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 11 2023 4, p 80
allfieldsGer	10.3390/galaxies11040080 doi (DE-627)DOAJ093614438 (DE-599)DOAJ38d0e648f00e47ad83183065fc2b836a DE-627 ger DE-627 rakwb eng QB1-991 Paula Esther Marchiano verfasserin aut A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems. techniques: spectroscopic stars: symbiotic, binaries stars: infrared Astronomy María Laura Arias verfasserin aut Michaela Kraus verfasserin aut Michalis Kourniotis verfasserin aut Andrea Fabiana Torres verfasserin aut Lydia Sonia Cidale verfasserin aut Marcelo Borges Fernandes verfasserin aut In Galaxies MDPI AG, 2013 11(2023), 4, p 80 (DE-627)730276740 (DE-600)2691049-4 20754434 nnns volume:11 year:2023 number:4, p 80 https://doi.org/10.3390/galaxies11040080 kostenfrei https://doaj.org/article/38d0e648f00e47ad83183065fc2b836a kostenfrei https://www.mdpi.com/2075-4434/11/4/80 kostenfrei https://doaj.org/toc/2075-4434 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 11 2023 4, p 80
allfieldsSound	10.3390/galaxies11040080 doi (DE-627)DOAJ093614438 (DE-599)DOAJ38d0e648f00e47ad83183065fc2b836a DE-627 ger DE-627 rakwb eng QB1-991 Paula Esther Marchiano verfasserin aut A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems. techniques: spectroscopic stars: symbiotic, binaries stars: infrared Astronomy María Laura Arias verfasserin aut Michaela Kraus verfasserin aut Michalis Kourniotis verfasserin aut Andrea Fabiana Torres verfasserin aut Lydia Sonia Cidale verfasserin aut Marcelo Borges Fernandes verfasserin aut In Galaxies MDPI AG, 2013 11(2023), 4, p 80 (DE-627)730276740 (DE-600)2691049-4 20754434 nnns volume:11 year:2023 number:4, p 80 https://doi.org/10.3390/galaxies11040080 kostenfrei https://doaj.org/article/38d0e648f00e47ad83183065fc2b836a kostenfrei https://www.mdpi.com/2075-4434/11/4/80 kostenfrei https://doaj.org/toc/2075-4434 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 11 2023 4, p 80
language	English
source	In Galaxies 11(2023), 4, p 80 volume:11 year:2023 number:4, p 80
sourceStr	In Galaxies 11(2023), 4, p 80 volume:11 year:2023 number:4, p 80
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	techniques: spectroscopic stars: symbiotic, binaries stars: infrared Astronomy
isfreeaccess_bool	true
container_title	Galaxies
authorswithroles_txt_mv	Paula Esther Marchiano @@aut@@ María Laura Arias @@aut@@ Michaela Kraus @@aut@@ Michalis Kourniotis @@aut@@ Andrea Fabiana Torres @@aut@@ Lydia Sonia Cidale @@aut@@ Marcelo Borges Fernandes @@aut@@
publishDateDaySort_date	2023-01-01T00:00:00Z
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callnumber-first	Q - Science
author	Paula Esther Marchiano
spellingShingle	Paula Esther Marchiano misc QB1-991 misc techniques: spectroscopic misc stars: symbiotic, binaries misc stars: infrared misc Astronomy A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars
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topic_title	QB1-991 A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars techniques: spectroscopic stars: symbiotic, binaries stars: infrared
topic	misc QB1-991 misc techniques: spectroscopic misc stars: symbiotic, binaries misc stars: infrared misc Astronomy
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title	A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars
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title_full	A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars
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author_browse	Paula Esther Marchiano María Laura Arias Michaela Kraus Michalis Kourniotis Andrea Fabiana Torres Lydia Sonia Cidale Marcelo Borges Fernandes
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title_sort	mini atlas of h-band spectra of southern symbiotic stars
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title_auth	A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars
abstract	Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems.
abstractGer	Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems.
abstract_unstemmed	Symbiotic stars are interacting binary systems composed of an evolved star (generally a late-type red giant) and a degenerate or dwarf companion in orbit close enough for mass transfer to occur. Understanding the status of the late-type star is important for developing binary models for the symbiotic systems as it affects the transfer of matter needed to activate the hot component. Infrared observations have been very useful in probing the nature of late-type stars in symbiotic systems. This work presents a set of symbiotic stars observed with SOAR/OSIRIS (<i<R</i<∼3000) in the H-band. We aimed to search for possible molecular circumstellar emission, to characterize the cool companion in these systems, and to confront the new findings with those obtained from the previous K-band classifications. We detected molecular emission from just one object, BI Cru, which displays the second-overtone CO-bands. To fit the observed photospheric CO absorption bands, we used the MARCS atmosphere models. We present our results as a mini atlas of symbiotic stars in the near-infrared region to facilitate the comparison among different observed symbiotic systems.
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container_issue	4, p 80
title_short	A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars
url	https://doi.org/10.3390/galaxies11040080 https://doaj.org/article/38d0e648f00e47ad83183065fc2b836a https://www.mdpi.com/2075-4434/11/4/80 https://doaj.org/toc/2075-4434
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A Mini Atlas of H-Band Spectra of Southern Symbiotic Stars

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