Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-26T05:03:17.388Z Has data issue: false hasContentIssue false

IRAS 03158+4227 - a ULIRG in a Widely Separated Pair of Galaxies

Published online by Cambridge University Press:  12 April 2016

Helmut Meusinger
Affiliation:
Thüringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
Bringfried Stecklum
Affiliation:
Thüringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
Jens Brunzendorf
Affiliation:
Thüringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present new deep optical images, optical spectroscopy, and high-resolution NIR images of IRAS 03158+4227, one of the most luminous ULIRGs from the IRAS 2 Jy sample. The data are best explained either by a multiple merger or by the assumption of a ULIRG triggered in an early phase of galaxy interaction.

Type
Part 2. Infrared and Submillimeter Surveys for AGN
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

Bekki, K. 2001, ApJ, 546, 189 Google Scholar
Borne, K.D., Bushouse, H., Lucas, R.A. et al. 2000, AJ, 529, L77 Google Scholar
Dinh-V-Trung, , Lo, K.Y., & Kim, D.-C. 2001, ApJ, 556, 141 Google Scholar
Meusinger, H., Stecklum, B., Theis, C. et al. 2001, A&A, in pressGoogle Scholar
Murphy, T.W., Armus, L., Matthews, K. et al. 1996, AJ, 111, 1045 Google Scholar