Herschel-PACS spectroscopic diagnostics of local ULIRGs: Conditions and kinematics in Markarian 231
Astronomy and Astrophysics 518:2 (2010)
Abstract:
In this first paper on the results of our Herschel PACS survey of local ultra luminous infrared galaxies (ULIRGs), as part of our SHINING survey of local galaxies, we present far-infrared spectroscopy of Mrk 231, the most luminous of the local ULIRGs, and a type 1 broad absorption line AGN. For the first time in a ULIRG, all observed far-infrared fine-structure lines in the PACS range were detected and all were found to be deficient relative to the far infrared luminosity by 1-2 orders of magnitude compared with lower luminosity galaxies. The deficits are similar to those for the mid-infrared lines, with the most deficient lines showing high ionization potentials. Aged starbursts may account for part of the deficits, but partial covering of the highest excitation AGN powered regions may explain the remaining line deficits. A massive molecular outflow, discovered in OH and 18OH, showing outflow velocities out to at least 1400 km s-1, is a unique signature of the clearing out of the molecular disk that formed by dissipative collapse during the merger. The outflow is characterized by extremely high ratios of 18O/16O suggestive of interstellar medium processing by advanced starbursts. © 2010 ESO.Weighing black holes using open-loop focus corrections for LGS-AO observations of galaxy nuclei at Gemini Observatory
Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 7736 (2010) 77365w-77365w-8
Limits on the quiescent radio emission from the black hole binaries GRO J1655-40 and XTE J1550-564
(2010)
SUPERNOVA 2009kf: AN ULTRAVIOLET BRIGHT TYPE IIP SUPERNOVA DISCOVERED WITH PAN-STARRS 1 AND GALEX
The Astrophysical Journal Letters American Astronomical Society 717:1 (2010) l52-l56
An excess of star-forming galaxies in the fields of high-redshift QSOs
\mnras 405 (2010) 2623-2638-2623-2638