The Surroundings of Disturbed, Active Galaxies

Abstract

The brightest apparent magnitude examples of ultra luminous infrared galaxies (ULIRG's) are studied here in X-ray, optical, infrared and radio wavelengths. It is is found that they have associated material reaching out to apparent diameters of the order of a degree on the sky. Gas, dust, X-ray material and quasars appear to be ejected from the active nuclei with all objects nearer than their redshift distances.

14 pages, Figs. 1-28 jpg and gif files

References in corpus (7)

• Radio Continuum Evidence for Outflow and Absorption in the Seyfert 1 Galaxy Markarian 231
• The Neutral Hydrogen Distribution in Merging Galaxies: Differences between Stellar and Gaseous Tidal Morphologies
• The Starburst in the Central Kiloparsec of Markarian 231
• The FIRST Sample of Ultraluminous Infrared Galaxies at High Redshift I. Sample and Near-IR Morphologies
• The Identification of Quasars Behind Elliptical Galaxies and Clusters of Galaxies
• Redshifts of Galaxies Around Arp 220 and Serendipitous Discovery of Three Star-Forming Dwarf Galaxies at Redshift $z\sim$ 0.5
• The Nature of the Diffuse Clumps and the X-ray Companion of Mrk 273

Cited by in corpus (3)

• X-ray Emitting QSOs Ejected from Arp 220
• On QSO Distances and Lifetimes in a Local Model
• Multi-band optical variability of a newly discovered twelve blazars sample from 2013-2019