Infrared and radio emission from II ZW 40 and other blue dwarf galaxies

Details Infrared and radio emission from II ZW 40 and other blue dwarf galaxies Infrared and radio emission from II ZW 40 and other blue dwarf galaxies

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308..620w&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 308, Sept. 15, 1986, p. 620-626.

Astronomy and Astrophysics

Astronomy

33

Dwarf Galaxies, Emission Spectra, Infrared Spectra, Radio Spectra, Astronomical Catalogs, Astronomical Photometry, Atmospheric Attenuation, Infrared Astronomy Satellite, Spiral Galaxies, Very Large Array (Vla)

Scientific paper

A survey was made of 22 blue dwarf galaxies with the Very Large Array, a good correspondence between the detectability of radio emission and presence in the IRAS Point-Source Catalog was found. New ground-based infrared observations of a number of these galaxies are presented, with an emphasis on II Zw 40 and Markarian 206. II Zw 40 has an infrared-to-blue luminosity ratio of 25, which is among the highest found in the IRAS minisurvey of galaxies; the high value is probably the result of dust extinction close to the source of emission. The radio continuum emission from II Zw 40 includes a strong nonthermal component.

Affiliated with

Also associated with

No associations

Rating

Infrared and radio emission from II ZW 40 and other blue dwarf galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Infrared and radio emission from II ZW 40 and other blue dwarf galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared and radio emission from II ZW 40 and other blue dwarf galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1290854