Spectral analysis of four surprisingly similar hot hydrogen-rich subdwarf O stars

Context. Post-extreme horizontal branch stars (post-EHB) are helium-shell burning objects evolving away from the EHB and contracting directly towards the white dwarf regime. While the stars forming the EHB have been extensively studied in the past, their hotter and more evolved progeny are not so we...

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Bibliographic Details
Main Authors: Latour, M., Chayer, P., Green, E. M., Irrgang, A., Fontaine, G.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: EDP SCIENCES S A 2018
Subjects:
Online Access:http://hdl.handle.net/10150/626530
http://arizona.openrepository.com/arizona/handle/10150/626530