USING Hα MORPHOLOGY AND SURFACE BRIGHTNESS FLUCTUATIONS TO AGE-DATE STAR CLUSTERS IN M83
暂无分享，去创建一个
The University of Toledo | Institute for Astronomy | M. Dopita | D. Calzetti | J. Holtzman | R. O’Connell | U. Washington | U. Virginia | N. University | -INAF | I. O. Astronomy | J. Silk | P. McCarthy | A. Walker | E. Young | M. Carollo | A. Saha | B. Whitmore | B. Balick | J. Trauger | Nasa Jpl | Aura | R. Chandar | R. Windhorst | U. Oxford | H. Bond | Nasa Ames Research Center | Carnegie Institution of Washington | R. Kimble | M. Mutchler | Noao | A. S. University | J. Frogel | A. N. University | C. T. I. Observatory | F. Paresce | M. Disney | U. Massachusetts | Hwihyun Kim | C. University | D. Hall | G. Center | I. D. F. Cosmica | C. Kaleida | Erick T. Young Space Telescope Science Institute | ETH-Zurich | R. O’Connell | Matt Stankiewicz