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arXiv · 2203.15289

Identification of new classical Be stars from the LAMOST MRS survey

Luqian Wang·Jiao Li·You Wu·Douglas R. Gies·Jin Zhong Liu·Chao Liu·Yanjun Guo·Xuefei Chen·Zhanwen Han
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Abstract

Be stars are B-type main-sequence stars that display broad Balmer emission lines in their spectra. Identification of Be population is essential to further examine the formation and evolutionary models. We report the detection of classical Be (CBe) stars from observations with the Large sky Area Multi-Object fiber Spectroscopic Telescope Medium Resolution Survey of Date Release 7 (LAMOST MRS DR7). We used a deep convolutional neural network, the ResNet, with an 18-layer module to examine the morphology of the H alpha profile. We identified 1,162 candidate Be stars from the collection of 2,260,387 spectra for 789,918 stars in the database. The ResNet network achieves a Be star classification accuracy of 99.5%. Among the detections, 151 of these are prior known Be stars cross-matched from the literature. By applying a three-step test, we identified 183 new CBe stars. We find that 41 CBe stars are members of known open clusters. Based upon an investigation of the kinematics of the identified CBe stars from the Gaia EDR3 astrometric solutions, we identified 16 new runaways. These new identifications will provide a reference for future follow-ups to further investigate their physical properties.

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Luqian Wang, Jiao Li, You Wu, Douglas R. Gies, Jin Zhong Liu, Chao Liu, Yanjun Guo, Xuefei Chen, Zhanwen Han. 2022-03-29. Identification of new classical Be stars from the LAMOST MRS survey. https://doi.org/10.3847/1538-4365%2Fac617a

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