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A Pair of Compact Red Galaxies at Redshift 2.38, Immersed in a 100 kpc Scale Ly-alpha Nebula

Authors
  • Francis, P. J.
  • Williger, G. M.
  • Collins, N. R.
  • Palunas, P.
  • Malumuth, E. M.
  • Woodgate, B. E.
  • Teplitz, H. I.
  • Smette, A.
  • Sutherland, R. S.
  • Danks, A. C.
  • Hill, R. S.
  • Lindler, D.
  • Kimble, R. A.
  • Heap, S. A.
  • Hutchings, J. B.
Type
Preprint
Publication Date
Feb 15, 2001
Submission Date
Feb 15, 2001
Identifiers
DOI: 10.1086/321417
arXiv ID: astro-ph/0102263
Source
arXiv
License
Unknown
External links

Abstract

We present Hubble Space Telescope (HST) and ground-based observations of a pair of galaxies at redshift 2.38, which are collectively known as 2142-4420 B1 (Francis et al. 1996). The two galaxies are both luminous extremely red objects (EROs), separated by 0.8 arcsec. They are embedded within a 100 kpc scale diffuse Ly-alpha nebula (or blob) of luminosity ~10^44 erg/s. The radial profiles and colors of both red objects are most naturally explained if they are young elliptical galaxies: the most distant yet found. It is not, however, possible 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 solar masses and ages of ~7x10^8 years. Both galaxies have color gradients: their centers are significantly bluer than their outer regions. The surface brightness of both galaxies is roughly an order of magnitude greater than would be predicted by the Kormendy relation. A chain of diffuse star formation extending 1 arcsec from the galaxies may be evidence that they are interacting or merging. The Ly-alpha nebula surrounding the galaxies shows apparent velocity substructure of amplitude ~ 700 km/s. We propose that the Ly-alpha emission from this nebula may be produced by fast shocks, powered either by a galactic superwind or by the release of gravitational potential energy.

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