The Extreme Compact Starburst in MRK 273

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

standard AAS format, 23 pages, 5 figures, fixed figure. To appear in ApJ Letters

Scientific paper

10.1086/312584

Images of neutral Hydrogen 21cm absorption and radio continuum emission at 1.4 GHz from Mrk 273 were made using the Very Long Baseline Array and Very Large Array. These images reveal a gas disk associated with the northern nuclear region with a diameter of 0.5'' (370 pc), at an inclination angle of 53deg. The radio continuum emission is composed of a diffuse component plus a number of compact sources. This morphology resembles those of nearby, lower luminosity starburst galaxies. These images provide strong support for the hypothesis that the luminosity of the northern source is dominated by an extreme compact starburst. The HI 21cm absorption shows an east-west gradient in velocity of 450 km/s across 0.3'' (220 pc), implying an enclosed mass of 2e9 M_solar, comparable to the molecular gas mass. The brightest of the compact sources may indicate radio emission from an active nucleus (AGN), but this source contributes only 3.8% to the total flux density of the northern nuclear region. The HI 21cm absorption toward the southeast radio nucleus suggests infall at 200 km/s on scales < 40 pc, and the southwest near IR nucleus is not detected in high resolution radio continuum images.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The Extreme Compact Starburst in MRK 273 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 The Extreme Compact Starburst in MRK 273, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Extreme Compact Starburst in MRK 273 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-227565

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.