Collision-induced galaxy formation: semi-analytical model and multiwavelength predictions
- 21 July 2003
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 343 (1) , 107-115
- https://doi.org/10.1046/j.1365-8711.2003.06643.x
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- The cosmological density of baryons from observations of 3He+ in the Milky WayNature, 2002
- The Nature of the Hard X-Ray Background Sources: Optical, Near-Infrared, Submillimeter, and Radio PropertiesThe Astronomical Journal, 2001
- Constraints on Cosmological Parameters from MAXIMA-1The Astrophysical Journal, 2000
- Resolving the Submillimeter Background: The 850 Micron Galaxy CountsThe Astrophysical Journal, 1999
- Submillimetre-wavelength detection of dusty star-forming galaxies at high redshiftNature, 1998
- The Evolution of the Global Star Formation History as Measured from the Hubble Deep FieldThe Astrophysical Journal, 1997
- A Massive Z = 0.088 Supercluster and Tests of Starburst Galaxy Evolution at the North Ecliptic PoleThe Astrophysical Journal, 1996
- The statistics of peaks of Gaussian random fieldsThe Astrophysical Journal, 1986
- Tidal interactions between spherical galaxiesThe Astrophysical Journal, 1985
- 21-cm line studies of spiral galaxies. II. The distribution and kinematics of neutral hydrogen in spiral galaxies of various morphological types.The Astronomical Journal, 1981