... We thus correct our total SFR by a factor of 5.25, for a total of 96M yrю1. ... 96 ф 34 ( Balogh & Morris 2000), 253 ф 34 ( Kodama et al. 2004), 78 ф 7 ( Finn et al. 2004), and 96 ф 24 M yrю1, respectively ...
... 1.16 Completed WF/PC-2 5415 (The Distance to M-96 Galaxy Group: Cycle 4 Medium) The WF/PC-2 was used to make observations of Cepheid variable stars within the galaxy NGC-3368 which itself is located in the M-96 galaxy cluster. ...
... Once the starting values are established, a stable outward integration method is employed to obtain the radial Ё For Sgr A , we adopt the values M = 2.6 в 106 M (Schodel et al. 2002) and M = 8.96 в 10-7 M yr-1 (Yuan et al. ...
... to the Extragalactic Reference Frame: BR12-23, Part 2) 3.13 Complete Two Sets of WF/PC-2 5415 (The Distance to the M-96 Galaxy Group: Cycle 4 Medium) 3.14 Complete WF/PC-2 5446 (The Nuclei of Nearby S0 and Spiral Galaxies: A PC Snapshot Imaging) 3.15 ...
... G.D. "HST time-resolved ultraviolet spectroscopy of ST LMi and UZ For: resolving the accretion stream" ApJ 10-1-96 CORBIN, M.R.; BOROSON, T.A. "Combined ultraviolet and optical spectra of 48 low-redshift QSOs and the relation of the continuum and emission ...