Hydrogen and Helium Shock Phenomena during Rising Light in RR Lyrae Fundamental Mode Pulsators

Author:

Preston George W.,Sneden ChristopherORCID,Chadid MeriemeORCID

Abstract

Abstract We present measurements of H and He emission and absorption lines produced in RRab fundamental mode pulsators during primary light rise. The lines define universal progressions of rise and decay in metal-poor RRab stars. Such a progression cannot be constructed for He in metal-rich RRab (those with [Fe/H] > −0.8) because weak He i emission is detected in only two of the six metal-rich RRab in our survey. Great variety exists in the phase variations of the blue- and red-shifted absorption components of the 5876 Å line during pre- and post-emission phases. Detection of measurable He ii 4686 Å emission in eight RRab, three of them Blazhko variables, provides an additional constraint on ionization of helium.

Funder

U.S. National Science Foundation

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The Van Hoof Effect over the Blazhko Cycle;The Astrophysical Journal;2023-07-01

2. The Active Chromospheres of Lithium-rich Red Giant Stars*;The Astrophysical Journal;2022-11-01

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