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37 papers · 2 filters
Molecular Gas Distribution in Double-Nucleus Ultraluminous Infrared Galaxies
A. S. Evans, J. A. Surace, J. M. Mazzarella +1
Millimeter (CO) observations of 5 double-nucleus ultraluminous infrared galaxy (ULIG) mergers are presented. With nuclear separations of 3-5 kpc, these galaxies are in the ``interm…
NICMOS Imaging of Infrared-Luminous Galaxies
N. Z. Scoville, A. S Evans, R. Thompson +6
We present near-infrared images obtained with the HST NICMOS camera for a sample of 9 luminous (LIGs: L_IR (8-1000 microns) >~ 10^11 L_sun) and 15 ultra-luminous (ULIGS: L_IR >~ 10…
The Origin of \lya Absorption Systems at ---Implications from the Hubble Deep Field
Hsiao-Wen Chen, Kenneth M. Lanzetta, Alberto Fernández-Soto
The Hubble Deep Field images have provided us with a unique chance to relate statistical properties of high-redshift galaxies to statistical properties of \lya absorption systems.…
Resolved CO(1-0) Nuclei in IRAS 14348-1447: Evidence for Massive Bulge Progenitors to Ultraluminous Infrared Galaxies
A. S. Evans, J. A. Surace, J. M. Mazzarella
High-resolution, CO(1-0) interferometry of the ultraluminous infrared galaxy IRAS 14348-1447 is presented. The merger system has a molecular gas mass of \~3x10^10 solar masses and…
Is Nova Sco 1994 (GRO 1655-40) a Relic of a GRB ?
G. E. Brown, C. -H. Lee, H. K. Lee +1
We suggest Nova Sco 1994 (GRO 1655-40) as a possible relic of a Gamma Ray Burster (GRB) and Type Ib supernova (SN) explosion, showing that there is evidence both that the black hol…
Numerical Models of Binary Neutron Star System Mergers. I.: Numerical Methods and Equilibrium Data for Newtonian Models
F. Douglas Swesty, Edward Y. M. Wang, Alan C. Calder
The numerical modeling of binary neutron star mergers has become a subject of much interest in recent years. While a full and accurate model of this phenomenon would require the ev…