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Title:
High spatial resolution continuum and H-alpha imaging of the high-redshift IRAS source FSC 10214+4724
Authors:
Soifer, B. T.; Neugebauer, G.; Matthews, K.; Lawrence, C.; Mazzarella, J.
Affiliation:
AA(Palomar Observatory, Pasadena, CA), AB(Palomar Observatory, Pasadena, CA), AC(Palomar Observatory, Pasadena, CA), AD(Palomar Observatory, Pasadena, CA), AE(California Inst. of Technology, Pasadena)
Publication:
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 399, no. 1, p. L55-L58. (ApJ Homepage)
Publication Date:
11/1992
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
GALACTIC EVOLUTION, H ALPHA LINE, INFRARED SOURCES (ASTRONOMY), INTERACTING GALAXIES, RED SHIFT, SPATIAL RESOLUTION, FAINT OBJECTS, INFRARED ASTRONOMY SATELLITE, LUMINOSITY, QUASARS
DOI:
10.1086/186605
Bibliographic Code:
1992ApJ...399L..55S

Abstract

New observations are reported which support the view that the high-redshift IRAS source FSC 10214+4724 is a rare extreme example of the class of ultraluminous infrared galaxies observed in the local universe. The presence of two continuum components and a compact H-alpha source suggests that a merger between two or more gas-rich systems has triggered the production of a powerful dust-enshrouded quasar which is responsible for the bulk of the luminosity.

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