Lost siblings of the Sun: Revisiting the FGK potential candidates

Details Lost siblings of the Sun: Revisiting the FGK potential candidates Lost siblings of the Sun: Revisiting the FGK potential candidates

Jul 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012newa...17..514b&link_type=abstract

New Astronomy, Volume 17, Issue 5, p. 514-519.

Astronomy and Astrophysics

Astronomy

Scientific paper

The main goal of this paper is to revisit the lost siblings of the Sun candidates within 100 pc. The solar siblings should have some similar characteristics as their ages, chemical compositions and kinematics properties. Considering their chemical compositions, age and kinematics properties only three potential candidates have been found in the literature: HD28676, HD83423 and HD175740. The first two stars are mentioned by Brown et al. (2010) and Bobylev et al. (2011), respectively. HD175740 is, to our knowledge, the first giant to be proposed as potential candidate.

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