Autor:	Bergh, Sidney van den
Rok vydání:	2012
Předmět:	Astrophysics - Astrophysics of Galaxies Astrophysics - Cosmology and Nongalactic Astrophysics
Druh dokumentu:	Working Paper
DOI:	10.1088/0004-637X/746/2/189
Popis:	A study is made of deviations from the mean power-law relationship between the Galactocentric distances and the half-light radii of Galactic globular clusters. Surprisingly, deviations from the mean R_h versus R_gc relationship do not appear to correlate with cluster luminosity, cluster metallicity, or horizontal branch morphology. Differences in orbit shape are found to contribute to the scatter in the R_h versus R_gc relationship of Galactic globular clusters. Comment: Accepted for publication in The Astrophysical Journal
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/1201.3597 Zobrazit plný text záznamu View this record from Arxiv