Search Publications

A Relationship Between Supermassive Black Hole Mass and the Total Gravitational Mass of the Host Galaxy
DOI: 10.1088/0004-637X/704/2/1135 Bibcode: 2009ApJ...704.1135B

Crampton, David; Simard, Luc; Bandara, Kaushala

We investigate the correlation between the mass of a central supermassive black hole (SMBH) and the total gravitational mass of the host galaxy (M tot). The results are based on 43 galaxy-scale strong gravitational lenses from the Sloan Lens ACS Surveys (SLACS) Survey whose black hole masses were estimated through two scaling relations:…

2009 The Astrophysical Journal
eHST 92
The Galactic Positron Annihilation Radiation and the Propagation of Positrons in the Interstellar Medium
DOI: 10.1088/0004-637X/698/1/350 Bibcode: 2009ApJ...698..350H

Rothschild, R. E.; Higdon, J. C.; Lingenfelter, R. E.

The ratio of the luminosity of diffuse 511 keV positron annihilation radiation, measured by INTEGRAL in its four years, from a Galactic "positron bulge" (<1.5 kpc) compared to that of the disk is ~1.4. This ratio is roughly 4 times larger than that expected simply from the stellar bulge-to-disk ratio of ~0.33 of the Galactic supernovae (SNe), w…

2009 The Astrophysical Journal
INTEGRAL 92
Galaxy Clusters in the Swift/Burst Alert Telescope Era: Hard X-rays in the Intracluster Medium
DOI: 10.1088/0004-637X/690/1/367 Bibcode: 2009ApJ...690..367A

Böhringer, H.; Greiner, J.; Moretti, A. +6 more

We report the detection of 10 clusters of galaxies in the ongoing Swift/Burst Alert Telescope (BAT) all-sky survey. This sample, which mostly comprises merging clusters, was serendipitously detected in the 15-55 keV band. We use the BAT sample to investigate the presence of excess hard X-rays above the thermal emission. The BAT clusters do not sho…

2009 The Astrophysical Journal
INTEGRAL XMM-Newton 92
Evidence of Widespread Hot Plasma in a Nonflaring Coronal Active Region from Hinode/X-Ray Telescope
DOI: 10.1088/0004-637X/698/1/756 Bibcode: 2009ApJ...698..756R

Testa, Paola; Reale, Fabio; Parenti, Susanna +1 more

Nanoflares, short and intense heat pulses within spatially unresolved magnetic strands, are now considered a leading candidate to solve the coronal heating problem. However, the frequent occurrence of nanoflares requires that flare-hot plasma be present in the corona at all times. Its detection has proved elusive until now, in part because the int…

2009 The Astrophysical Journal
Hinode 92
The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
DOI: 10.1088/0004-637X/698/2/1963 Bibcode: 2009ApJ...698.1963R

Roederer, Ian U.; Frebel, Anna; Christlieb, Norbert +4 more

We examine the Pb and Th abundances in 27 metal-poor stars (-3.1< [Fe/H] <-1.4) whose very heavy metal (Z > 56) enrichment was produced only by the rapid (r-) nucleosynthesis process. New abundances are derived from Hubble Space Telescope/Space Telescope Imaging Spectrograph, Keck/High Resolution Echelle Spectrograph, and Very Large Teles…

2009 The Astrophysical Journal
eHST 91
Hinode X-Ray Telescope Detection of Hot Emission from Quiescent Active Regions: A Nanoflare Signature?
DOI: 10.1088/0004-637X/693/2/L131 Bibcode: 2009ApJ...693L.131S

Klimchuk, J. A.; Golub, L.; Schmelz, J. T. +4 more

The X-Ray Telescope (XRT) on the Japanese/USA/UK Hinode (Solar-B) spacecraft has detected emission from a quiescent active region core that is consistent with nanoflare heating. The fluxes from 10 broadband X-ray filters and filter combinations were used to construct differential emission measure (DEM) curves. In addition to the expected active re…

2009 The Astrophysical Journal
Hinode 91
Imaging The Molecular Gas in a z = 3.9 Quasar Host Galaxy at 0farcs3 Resolution: A Central, Sub-Kiloparsec Scale Star Formation Reservoir in APM 08279+5255
DOI: 10.1088/0004-637X/690/1/463 Bibcode: 2009ApJ...690..463R

Lewis, Geraint F.; Walter, Fabian; Carilli, Christopher L. +1 more

We have mapped the molecular gas content in the host galaxy of the strongly lensed high-redshift quasar APM 08279+5255 (z = 3.911) with the Very Large Array at 0farcs3 resolution. The CO(J = 1 → 0) emission is clearly resolved in our maps. The CO(J = 1 → 0) line luminosity derived from these maps is in good agreement with a previous single-dish me…

2009 The Astrophysical Journal
eHST 91
Calibration Of [O IV] 26 µm as a Measure of Intrinsic Active Galactic Nucleus Luminosity
DOI: 10.1088/0004-637X/700/2/1878 Bibcode: 2009ApJ...700.1878R

Rigby, J. R.; Aniano, G.; Diamond-Stanic, A. M.

We compare [O IV] 25.89 µm emission line luminosities with very hard (10-200 keV) X-rays from Swift, INTEGRAL, and BeppoSAX for a complete sample of 89 Seyferts from the Revised Shapley-Ames sample. Using Seyfert 1s, we calibrate [O IV] as a measure of active galactic nucleus (AGN) intrinsic luminosity, for particular use in high-obscuration…

2009 The Astrophysical Journal
INTEGRAL 90
The UDF05 Follow-Up of the Hubble Ultra Deep Field. II. Constraints on Reionization from Z-Dropout Galaxies
DOI: 10.1088/0004-637X/690/2/1350 Bibcode: 2009ApJ...690.1350O

Panagia, N.; Gardner, Jonathan P.; Ferguson, H. C. +12 more

We detect three (plus one less certain) z 850-dropout sources in two separate fields (Hubble Ultra Deep Field and NICP34) of our UDF05 Hubble Space Telescope Near-Infrared Camera and Multi-Object Spectrometer images. These z ~ 7 Lyman-break Galaxy (LBG) candidates allow us to constrain the Luminosity Function (LF) of the star-forming ga…

2009 The Astrophysical Journal
eHST 90
The Evolution Of Massive Young Stellar Objects in the Large Magellanic Cloud. I. Identification and Spectral Classification
DOI: 10.1088/0004-637X/699/1/150 Bibcode: 2009ApJ...699..150S

Brandner, Wolfgang; Chu, You-Hua; Gruendl, Robert A. +5 more

We present and categorize Spitzer infrared spectrometer spectra of 294 objects in the Large Magellanic Cloud (LMC) to create the largest and most complete catalog of massive young stellar object (YSO) spectra in the LMC. Target sources were identified from infrared photometry and multiwavelength images indicative of young, massive stars highly ens…

2009 The Astrophysical Journal
ISO 89