2001/02/15 by Paul Francis, P. J. Francis, G. M. Williger +21 · 1 citation
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.1086/321417
33 pages, 9 figures, ApJ in press (to appear in Jun 10 issue)
arxiv created 2001/02/15 · openalex publication_date 2001/06/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31
We present Hubble Space Telescope and ground-based observations of a pair of galaxies at a redshift of 2.38, which are collectively known as 2142-4420 B1. Both galaxies are luminous extremely red objects (EROs) and are separated by 0 8. They are embedded within a 100 kpc scale diffuse Lyα nebula (or blob) of luminosity ~10 44 ergs s -1 . The radial profiles and colors of both red objects are most naturally explained if they are young elliptical galaxies, the most distant galaxies of this type found to date. It is not possible, however, to rule out a model in which they are abnormally compact, extremely dusty starbursting disk galaxies. If they are elliptical galaxies, their stellar populations have inferred masses of ~10 11 M ☉ and ages of ~7 × 10 8 yr. Both galaxies have color gradients: their centers are significantly bluer than their outer regions. The surface brightness of both galaxies is roughly 1 order of magnitude greater than would be predicted by the Kormendy relation. A chain of diffuse star formation extending 1'' from the galaxies may be evidence that they are interacting or merging. The Lyα nebula surrounding the galaxies shows apparent velocity substructure of amplitude ~700 km s -1 . We propose that the Lyα emission from this nebula may be produced by fast shocks that are powered either by a galactic superwind or by the release of gravitational potential energy.