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Konkoly optical catalog of young stars for the Gaia Photometric Science Alerts

Published online by Cambridge University Press:  13 January 2020

E. Varga-Verebélyi
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
M. Kun
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
E. Szegedi-Elek
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
P. Ábrahám
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
J. Varga
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
Cs. Kiss
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
Á. Kóspál
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
G. Marton
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
L. Szabados
Affiliation:
Konkoly Observatory, Konkoly Thege Miklós út 15-17, H-1121 Budapest, Hungary email: [email protected]
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Abstract

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Our aim is to present a new and so far most complete catalog of optically selected young stars. The basis of this work is an extensive literature search for young stars in all the known nearby (< 2 kpc) star forming regions, included in the Handbook of Star Forming Regions [4, 5], and in 67 additional catalogs. We collected data on known young, pre-main-sequence stars detected in optical bands. The catalog contains the celestial coordinates, object names, names of the enclosing star forming region, identification methods, distances, and other information (e.g., references, binarity) for 15208 young stellar objects. It is already in use by the Gaia Photometric Science Alerts Team to identify variable young stars in the Gaia data. Our catalog was cross-correlated with the Gaia DR2 and we obtained flux and distance estimations for 86% of the stars.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020 

References

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