The extreme compact starburst in Markarian 273

Citation
Cl. Carilli et Gb. Taylor, The extreme compact starburst in Markarian 273, ASTROPHYS J, 532(2), 2000, pp. L95-L99
Citations number
41
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
532
Issue
2
Year of publication
2000
Part
2
Pages
L95 - L99
Database
ISI
SICI code
0004-637X(20000401)532:2<L95:TECSIM>2.0.ZU;2-G
Abstract
Images of neutral hydrogen 21 cm 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 n uclear region with a diameter 0."5 (370 pc) at an inclination angle of 53 d egrees. The radio continuum emission is composed of a diffuse component plu s a number of compact sources. This morphology resembles those of nearby, l ower 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 H I 21 cm absorption shows an east-west g radient in velocity of 450 km s(-1) across 0."3 (220 pc), which implies an enclosed mass of 2 x 10(9) M-circle dot, comparable to the molecular gas ma ss. The brightest of the compact sources may indicate radio emission from a n active nucleus, but this source contributes only 3.8% to the total flux d ensity of the northern nuclear regions. The H I 21 cm absorption toward the southeast radio nucleus suggests infall at 200 km s(-1) on scales less tha n or equal to 40 pc, and the southwest near-LR nucleus is not detected in h igh-resolution radio continuum images.