COLA. III. RADIO DETECTION OF ACTIVE GALACTIC NUCLEUS IN COMPACT MODERATE LUMINOSITY INFRARED GALAXIES

Journal Article · Wed Sep 01 04:00:00 EDT 2010 · Astrophysical Journal

DOI:https://doi.org/10.1088/0004-637X/720/1/555· OSTI ID:21460099

Parra, R; Conway, J E; Aalto, S ^[1]; Appleton, P N ^[2]; Norris, R P ^[3]; Pihlstroem, Y M ^[4]; Kewley, L J ^[5]

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1. Onsala Space Observatory, SE-439 92 Onsala (Sweden)
2. NASA Herschel Science Center, Mail Code 100-22, California Institute of Technology. 770 S. Wilson Blvd., Pasadena, CA 91125 (United States)
3. CSIRO Australia Telescope National Facility, P.O. Box 76, Epping, NSW 1710 (Australia)
4. Department of Physics and Astronomy, UNM, 800 Yale Blvd., NE, Albuquerque, NM 87131 (United States)
5. University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

We present results from 4.8 GHz Very Large Array (VLA) and global very long baseline interferometry (VLBI) observations of the northern half of the moderate FIR luminosity (median L{sub IR} = 10{sup 11.01} L{sub sun}) COLA sample of star-forming galaxies. VLBI sources are detected in a high fraction (20/90) of the galaxies observed. The radio luminosities of these cores ({approx}10{sup 21} W Hz{sup -1}) are too large to be explained by radio supernovae or supernova remnants and we argue that they are instead powered by active galactic nuclei (AGNs). These sub-parsec scale radio cores are preferentially detected toward galaxies whose VLA maps show bright 100-500 parsec scale nuclear radio components. Since these latter structures tightly follow the FIR to radio-continuum correlation for star formation, we conclude that the AGN-powered VLBI sources are associated with compact nuclear starburst environments. The implications for possible starburst-AGN connections are discussed. The detected VLBI sources have a relatively narrow range of radio luminosity consistent with models in which intense compact Eddington-limited starbursts regulate the gas supply onto a central supermassive black hole. The high incidence of AGN radio cores in compact starbursts suggests little or no delay between the starburst phase and the onset of AGN activity.

• OSTI ID: 21460099
• Journal Information: Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 720; ISSN ASJOAB; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
BINARY STARS
BLACK HOLES
COSMIC RADIO SOURCES
ERUPTIVE VARIABLE STARS
GALAXIES
GALAXY NUCLEI
INTERFEROMETRY
LUMINOSITY
OPTICAL PROPERTIES
PHYSICAL PROPERTIES
STARS
SUPERNOVA REMNANTS
SUPERNOVAE
VARIABLE STARS