Subaru and Salt Spectroscopy of Chemically Peculiar Hot Subdwarfs

The majority of hot subdwarfs lie on or close to the helium main-sequence. Many have hydrogen-rich surfaces, but a substantial fraction of the hotter subdwarfs have hydrogen-depleted or hydrogen-deficient surfaces. Amongst the former, three were known to show extraordinary overabundances of heavy el...

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Bibliographic Details
Main Authors: Jeffery C. Simon, Neelamkodan Naslim, Woolf Vincent M., Crawford Steven M., Østensen Roy H.
Format: Article
Language:English
Published: De Gruyter 2017-12-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0439