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arXiv · 1306.3754

Hydrogen lines in LAMOST low resolution spectra of RR Lyrae stars

F. Yang·L. Deng·C. Liu·J. L. Carlin·H. Jo Newberg·K. Carrell·X. Zhang·Z. Bai·F. Wang·H. Zhang·K. Wang·Y. Xin·Y. Xu·S. Gao·Y. Zhang·J. Li·Y Zhao
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Abstract

The LAMOST spectroscopic survey for Galactic structure and evolution has been in operation since October 2012, following a one-year pilot survey. The pilot survey produced a data release containing over 600,000 stellar spectra. By cross-checking with a large time series photometric database of RR Lyrae stars in high Galactic latitude regions, we found a total number of 157 stars that have been observed with LAMOST. In this sample, we successfully captured three RR Lyrae stars in the fast expansion phase, all of them showing significant hypersonic shock wave features in the spectra. By fitting the Hα line shape, we determine that the emission features seen within the broader Hα absorption line suggest hypersonic relative motions in the atmospheres of these three objects. With a further LAMOST survey of millions of stars, we will capture a large sample of RR Lyrae stars in their hypersonic expansion phase, and therefore provide a large database for the study of the internal structure and pulsation mechanism of RR Lyrae stars.

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F. Yang, L. Deng, C. Liu, J. L. Carlin, H. Jo Newberg, K. Carrell, X. Zhang, Z. Bai, F. Wang, H. Zhang, K. Wang, Y. Xin, Y. Xu, S. Gao, Y. Zhang, J. Li, Y Zhao. 2013-06-20. Hydrogen lines in LAMOST low resolution spectra of RR Lyrae stars. https://doi.org/10.1016/j.newast.2013.06.002

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