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26 April 2024
 
  » arxiv » astro-ph/9612153

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Pre-Starbursts in Luminous IR Galaxies ?
Yu Gao ; Robert A. Gruendl ; K.Y. Lo ; C.Y. Hwang ; S. Veilleux ;
Date 16 Dec 1996
Subject astro-ph
AffiliationLab. for Astronomical Imaging, Univ. of Illinois), C.Y. Hwang (ASIAA, Taiwan), and S. Veilleux (U. of Maryland
AbstractWe present first results of our on-going BIMA Key Project: imaging the CO(1-0) emission from a sample of 10 luminous IR galaxies (LIRGs) that are at various merging stages, with special emphasis on systems apparently in the early/intermediate stages of merging. We present here CO images with $sim 5’’$ resolution. An important result is the recognition of a plausible pre-starburst phase in some early LIRG mergers (e.g., Arp 302 and NGC 6670). Our initial analysis suggests that a merger-induced starburst phase may not begin before the nuclear separation between the merging galaxies reaches roughly 10 kpc. The surface gas density seems to increase from a few times $10^2 Msun pc^{-2} to >10^3 Msun pc^{-2}$ while the prominent CO extent systematically decreases as merging progresses.
Source arXiv, astro-ph/9612153
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