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The GALAH survey : A catalogue of carbon-enhanced stars and CEMP candidates

Cotar, Klemen (author)
University of Ljubljana
Zwitter, Tomaz (author)
University of Ljubljana
Kos, Janez (author)
University of Sydney,University of Ljubljana
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Munari, Ulisse (author)
INAF - Osservatorio Astronomico di Padova
Martell, Sarah L. (author)
University of New South Wales
Asplund, Martin (author)
Australian National University
Bland-Hawthorn, Joss (author)
University of Sydney
Buder, Sven (author)
Max Planck Institute for Astronomy
De Silva, Gayandhi M. (author)
Macquarie University, Sydney
Freeman, Kenneth C. (author)
Australian National University
Sharma, Sanjib (author)
University of Sydney
Anguiano, Borja (author)
University of Virginia
Carollo, Daniela (author)
National Institute for Astrophysics
Horner, Jonathan (author)
University of Southern Queensland
Lewis, Geraint F. (author)
University of Sydney
Nataf, David M. (author)
Johns Hopkins University
Nordlander, Thomas (author)
Australian National University
Stello, Denis (author)
University of Sydney
Ting, Yuan Sen (author)
Princeton University,Institute for Advanced Study, Princeton,Carnegie Observatories
Tinney, Chris (author)
University of New South Wales
Traven, Gregor (author)
Lund University,Lunds universitet,Astronomi - Genomgår omorganisation,Institutionen för astronomi och teoretisk fysik - Genomgår omorganisation,Naturvetenskapliga fakulteten,Lund Observatory - Undergoing reorganization,Department of Astronomy and Theoretical Physics - Undergoing reorganization,Faculty of Science,University of Ljubljana
Wittenmyer, Rob A. (author)
University of Southern Queensland
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 (creator_code:org_t)
 
2018-11-22
2019
English 17 s.
In: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 483:3, s. 3196-3212
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Swan bands-characteristic molecular absorption features of the C2 molecule-are a spectroscopic signature of carbon-enhanced stars. They can also be used to identify carbonenhanced metal-poor (CEMP) stars. The GALAH (GALactic Archaeology with Hermes) is a magnitude-limited survey of stars producing high-resolution, high-signal-to-noise spectra. We used 627 708 GALAH spectra to search for carbon-enhanced stars with a supervised and unsupervised classification algorithm, relying on the imprint of the Swan bands. We identified 918 carbon-enhanced stars, including 12 already described in the literature. An unbiased selection function of the GALAH survey allows us to perform a population study of carbon-enhanced stars. Most of them are giants, out of which we find 28 CEMP candidates. A large fraction of our carbon-enhanced stars with repeated observations show variation in radial velocity, hinting that there is a large fraction of variables among them. 32 of the detected stars also show strong Lithium enhancement in their spectra.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

Keyword

Catalogues
Methods: data analysis
Stars: abundances
Stars: carbon

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