English

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

Astrophysics 2009-11-06 v1

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.

Keywords

Cite

@article{arxiv.astro-ph/0102263,
  title  = {A Pair of Compact Red Galaxies at Redshift 2.38, Immersed in a 100 kpc Scale Ly-alpha Nebula},
  author = {P. J. Francis and G. M. Williger and N. R. Collins and P. Palunas and E. M. Malumuth and B. E. Woodgate and H. I. Teplitz and A. Smette and R. S. Sutherland and A. C. Danks and R. S. Hill and D. Lindler and R. A. Kimble and S. A. Heap and J. B. Hutchings},
  journal= {arXiv preprint arXiv:astro-ph/0102263},
  year   = {2009}
}

Comments

33 pages, 9 figures, ApJ in press (to appear in Jun 10 issue)