Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus

Spectral and luminosity classes, absolute magnitudes, color excesses, interstellar extinctions and distances are determined for 98 stars down to 18 mag in the Barnard 1 dark cloud belonging to the Per OB2 association. The classification of stars is based on their photoelectric photometry in the Viln...

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Main Authors: Černis K., Straižys V.
Format: Article
Language:English
Published: De Gruyter 2003-09-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0054
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spelling doaj-398387610f874ebf831f32161a6a87ad2021-09-06T19:40:11ZengDe GruyterOpen Astronomy2543-63762003-09-0112330132110.1515/astro-2017-0054astro-2017-0054Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in PerseusČernis K.0Straižys V.1Institute of Theoretical Physics and Astronomy, Vilnius University, Goštauto 12, Vilnius 2600, LithuaniaInstitute of Theoretical Physics and Astronomy, Vilnius University, Goštauto 12, Vilnius 2600, LithuaniaSpectral and luminosity classes, absolute magnitudes, color excesses, interstellar extinctions and distances are determined for 98 stars down to 18 mag in the Barnard 1 dark cloud belonging to the Per OB2 association. The classification of stars is based on their photoelectric photometry in the Vilnius seven-color photometric system. The extinction vs. distance diagram exhibits the presence of two dust layers at 150 and 230 pc distances. The distance of the first cloud, which gives an extinction Ay of 0.3 mag, coincides with the distance of the Taurus dark cloud complex. The second cloud with much larger extinction is about at the same distance as the clouds in the direction of the nearby objects: reflection nebula NGC 1333 and open cluster IG 348.https://doi.org/10.1515/astro-2017-0054techniquesphotometricvilnius photometric system-starsfundamental parametersclassification ismextinctiondust clouds ismindividual objectsbarnard 1
collection DOAJ
language English
format Article
sources DOAJ
author Černis K.
Straižys V.
spellingShingle Černis K.
Straižys V.
Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
Open Astronomy
techniques
photometric
vilnius photometric system-stars
fundamental parameters
classification ism
extinction
dust clouds ism
individual objects
barnard 1
author_facet Černis K.
Straižys V.
author_sort Černis K.
title Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
title_short Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
title_full Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
title_fullStr Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
title_full_unstemmed Interstellar Extinction in the Direction of The Barnard 1 Dark Cloud in Perseus
title_sort interstellar extinction in the direction of the barnard 1 dark cloud in perseus
publisher De Gruyter
series Open Astronomy
issn 2543-6376
publishDate 2003-09-01
description Spectral and luminosity classes, absolute magnitudes, color excesses, interstellar extinctions and distances are determined for 98 stars down to 18 mag in the Barnard 1 dark cloud belonging to the Per OB2 association. The classification of stars is based on their photoelectric photometry in the Vilnius seven-color photometric system. The extinction vs. distance diagram exhibits the presence of two dust layers at 150 and 230 pc distances. The distance of the first cloud, which gives an extinction Ay of 0.3 mag, coincides with the distance of the Taurus dark cloud complex. The second cloud with much larger extinction is about at the same distance as the clouds in the direction of the nearby objects: reflection nebula NGC 1333 and open cluster IG 348.
topic techniques
photometric
vilnius photometric system-stars
fundamental parameters
classification ism
extinction
dust clouds ism
individual objects
barnard 1
url https://doi.org/10.1515/astro-2017-0054
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