Model Spectra of Hot Subdwarfs for the Gaia Mission

Luke Hindson, R. Napiwotzki, U. Heber, M. Lemke

Research output: Chapter in Book/Report/Conference proceedingConference contribution

49 Downloads (Pure)

Abstract

The Gaia mission will provide an unprecedented 3D view of our galaxy, it will obtain astrometric, photometric and spectrographic data for roughly one billion stars. We are particularly interested in the treasure chest of new data Gaia will produce for hot subdwarf B (sdB) stars. In order for Gaia to classify sdBs and estimate parameters model spectra covering a wide parameter range are needed. Here we describe the construction of an extensive grid, which will be used for this purpose.
Original languageEnglish
Title of host publicationIn: Hot Subdwarf Stars and Related Objects - ASP Conference Series 392
PublisherAstronomical Society of the Pacific
Pages163-166
ISBN (Print)978-1-58381-654-7, 978-1-58381-655-4
Publication statusPublished - 2008

Fingerprint

Dive into the research topics of 'Model Spectra of Hot Subdwarfs for the Gaia Mission'. Together they form a unique fingerprint.

Cite this