The Value-added Catalog of OB Stars in LAMOST DR7

Abstract In this work, we update the catalog of OB stars based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope data release 7 and modify the OB stars’ selection criteria in spectral line indices’ space. The new catalog includes 37,778 spectra of 27,643 OB stars, of which 3827 OB stars are newly identified. The spectral subclasses of 27,643 OB stars are obtained using the automatic classification code MKCLASS. We find that the modified OB star selection criteria can better improve the completeness of late B-type stars by analyzing their spectral classification results given by MKCLASS. We also identify 3006 Be-type stars or candidates by examining the Balmer lines in their spectra and find that the frequency of our Be-type stars (10.9%) is consistent with previous results. The spatial distribution of OB stars indicates that they are mainly located in the Galactic disk. This new catalog of OB stars will provide valuable data for studying the structure and evolution of the Milky Way.

Authors

Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2024-11-13
DOI
https://doi.org/10.3847/1538-4365/ad833f
Citations
3
Primary Topic
Astronomical Observations and Instrumentation
Type
article
Field-Weighted Citation Impact
1.12

Funders

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article

The Value-added Catalog of OB Stars in LAMOST DR7

Zhenyan Huo, Jianrong Shi, Guozhen Hu, Wenyuan Cui et al.
3 citations
The Astrophysical Journal Supplement Series
Astronomical Observations and Instrumentation
1.12
article

The Value-added Catalog of OB Stars in LAMOST DR7

Zhenyan Huo, Jianrong Shi, Guozhen Hu, Wenyuan Cui, Xiao-Long Wang, Zhicun Liu, Jiaying Gu
article en
3 citations

Abstract

Abstract In this work, we update the catalog of OB stars based on the Large Sky Area Multi-Object Fiber Spectroscopic Telescope data release 7 and modify the OB stars’ selection criteria in spectral line indices’ space. The new catalog includes 37,778 spectra of 27,643 OB stars, of which 3827 OB stars are newly identified. The spectral subclasses of 27,643 OB stars are obtained using the automatic classification code MKCLASS. We find that the modified OB star selection criteria can better improve the completeness of late B-type stars by analyzing their spectral classification results given by MKCLASS. We also identify 3006 Be-type stars or candidates by examining the Balmer lines in their spectra and find that the frequency of our Be-type stars (10.9%) is consistent with previous results. The spatial distribution of OB stars indicates that they are mainly located in the Galactic disk. This new catalog of OB stars will provide valuable data for studying the structure and evolution of the Milky Way.

The Astrophysical Journal Supplement SeriesVol. 275(2)
National Natural Science Foundation of China, Hebei Normal University, Natural Science Foundation of Hebei Province, Hebei Provincial Department of Bureau of Science and Technology
Openalex Percentile: Top 25%
Astronomical Observations and Instrumentation
1.12
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