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Results 1 - 4 of 4

Could Segue 1 be a destroyed star cluster? - a dynamical perspective. (arXiv:1606.08778v1 [astro-ph.GA])
- Volume 11, Issue 27 - article #3
- Raul Dominguez (1), Michael Fellhauer (1), Matias Blaña (2), Juan-Pablo Farias (1,4), Jörg Dabringhausen (1), Graeme N. Candlish (1,5), Rory Smith (3), Nelvy Choque (1) ((1) Departamento de Astronomia, Universidad de Concepcion, Chile, (2) Max-Planck-Institut für extraterrestrische Physik, Garching, Germany, (3) Yonsei University, Seoul, Republic of Corea, (4) University of Florida, USA, (5) Universidad de Valparaiso, Chile)
- http://arxiv.org/abs/1606.08778
A Formation Scenario for the Disk of Satellites: Accretion of Satellites during Mergers
- Volume 11, Issue 9 - article #9
- Rory Smith, Pierre Alain Duc, Frederic Bournaud, and Sukyoung K. Yi
- The Astrophysical Journal - Volume: 818, Issue: 1
- View article PDF (2.34 MB)
Origin of the Metallicity Distribution in the Thick Disc
- Volume 10, Issue 46 - article #14
- Maider S. Miranda, Kate Pilkington, Brad K. Gibson, Christopher B. Brook, Patricia Sánchez-Blázquez, Ivan Minchev, Christopher Gareth Few, Rory Smith, Rosa Domínguez-Tenreiro, Aura Obreja, Jeremy Bailin, Greg S. Stinson
- arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Dec
- arXiv:1512.04559 [pdf]
Leo IV & V - A possible dwarf galaxy pair ?
- Volume 7, Issue 14 - article #6
- Matias Blaña (1), Michael Fellhauer (1), Rory Smith (1) ((1) Departamento de Astronomía, Universidad de Concepción)
- arXiv.org - Astrophysics - Volume: 2012, Issue: 6 Apr
- arXiv:1204.1285 [pdf, ps, other]

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