Search Publications

GREAT confirms transient nature of the circum-nuclear disk
DOI: 10.1051/0004-6361/201219068 Bibcode: 2012A&A...542L..21R

Martín-Pintado, J.; Harris, A. I.; Stutzki, J. +6 more

We report SOFIA/GREAT, Herschel/HIFI, and ground-based velocity-resolved spectroscopy of carbon monoxide (CO) rotational transitions from J = 2-1 to J = 16-15 toward two positions in the circum-nuclear disk (CND) in our Galactic center. Radiative transfer models were used to derive information on the physical state of the gas traced by CO. The exc…

2012 Astronomy and Astrophysics
Herschel 80
Red and Dead: The Progenitor of SN 2012aw in M95
DOI: 10.1088/2041-8205/759/1/L13 Bibcode: 2012ApJ...759L..13F

Sollerman, J.; Inserra, C.; Smartt, S. J. +17 more

Core-collapse supernovae (SNe) are the spectacular finale to massive stellar evolution. In this Letter, we identify a progenitor for the nearby core-collapse SN 2012aw in both ground-based near-infrared and space-based optical pre-explosion imaging. The SN itself appears to be a normal Type II Plateau event, reaching a bolometric luminosity of 10<…

2012 The Astrophysical Journal
eHST 80
Spatially Resolved Stellar, Dust, and Gas Properties of the Post-interacting Whirlpool Galaxy System
DOI: 10.1088/0004-637X/755/2/165 Bibcode: 2012ApJ...755..165M

Lebouteiller, Vianney; Wilson, Christine D.; Baes, Maarten +15 more

Using infrared imaging from the Herschel Space Observatory, observed as part of the Very Nearby Galaxies Survey, we investigate the spatially resolved dust properties of the interacting Whirlpool galaxy system (NGC 5194 and NGC 5195), on physical scales of ~1 kpc. Spectral energy distribution modeling of the new infrared images in combination with…

2012 The Astrophysical Journal
Herschel 80
Hot Disks and Delayed Bar Formation
DOI: 10.1088/0004-637X/758/2/136 Bibcode: 2012ApJ...758..136S

Weiner, Benjamin J.; Abraham, Roberto G.; Elmegreen, Bruce G. +4 more

We present observational evidence for the inhibition of bar formation in dispersion-dominated (dynamically hot) galaxies by studying the relationship between galactic structure and host galaxy kinematics in a sample of 257 galaxies between 0.1 < z <= 0.84 from the All-Wavelength Extended Groth Strip International Survey and the Deep Extragal…

2012 The Astrophysical Journal
eHST 79
The Submillimeter and Millimeter Excess of the Small Magellanic Cloud: Magnetic Dipole Emission from Magnetic Nanoparticles?
DOI: 10.1088/0004-637X/757/1/103 Bibcode: 2012ApJ...757..103D

Hensley, Brandon; Draine, B. T.

The Small Magellanic Cloud (SMC) has surprisingly strong submillimeter- and millimeter-wavelength emission that is inconsistent with standard dust models, including those with emission from spinning dust. Here, we show that the emission from the SMC may be understood if the interstellar dust mixture includes magnetic nanoparticles, emitting magnet…

2012 The Astrophysical Journal
Planck 79
Vertical profiling of SO 2 and SO above Venus' clouds by SPICAV/SOIR solar occultations
DOI: 10.1016/j.icarus.2011.09.025 Bibcode: 2012Icar..217..740B

Montmessin, Franck; Belyaev, Denis A.; Fedorova, Anna A. +6 more

New measurements of sulfur dioxide (SO 2) and monoxide (SO) in the atmosphere of Venus by SPICAV/SOIR instrument onboard Venus Express orbiter provide ample statistics to study the behavior of these gases above Venus' clouds. The instrument (a set of three spectrometers) is capable to sound atmospheric structure above the clouds in seve…

2012 Icarus
VenusExpress 79
Black Hole Powered Nebulae and a Case Study of the Ultraluminous X-Ray Source IC 342 X-1
DOI: 10.1088/0004-637X/749/1/17 Bibcode: 2012ApJ...749...17C

Feng, Hua; Grisé, Fabien; Kaaret, Philip +6 more

We present new radio, optical, and X-ray observations of three ultraluminous X-ray sources (ULXs) that are associated with large-scale nebulae. We report the discovery of a radio nebula associated with the ULX IC 342 X-1 using the Very Large Array (VLA). Complementary VLA observations of the nebula around Holmberg II X-1, and high-frequency Austra…

2012 The Astrophysical Journal
eHST 79
Modelling the huge, Herschel-resolved debris ring around HD 207129
DOI: 10.1051/0004-6361/201117731 Bibcode: 2012A&A...537A.110L

Magain, P.; Krivov, A. V.; Eiroa, C. +18 more

Debris disks, which are inferred from the observed infrared excess to be ensembles of dust, rocks, and probably planetesimals, are common features of stellar systems. As the mechanisms of their formation and evolution are linked to those of planetary bodies, they provide valuable information. The few well-resolved debris disks are even more valuab…

2012 Astronomy and Astrophysics
AKARI Herschel 79
Orion revisited. I. The massive cluster in front of the Orion nebula cluster
DOI: 10.1051/0004-6361/201220119 Bibcode: 2012A&A...547A..97A

Bouy, H.; Alves, J.


Aims: The aim of this work is to characterize the stellar population between Earth and the Orion A molecular cloud where the well-known star formation benchmark Orion nebula cluster (ONC) is embedded.
Methods: We used the denser regions the Orion A cloud to block optical background light, effectively isolating the stellar population in f…

2012 Astronomy and Astrophysics
XMM-Newton 79
Interstellar H I and H2 in the Magellanic Clouds: An Expanded Sample Based on Ultraviolet Absorption-line Data
DOI: 10.1088/0004-637X/745/2/173 Bibcode: 2012ApJ...745..173W

Welty, Daniel E.; Wong, Tony; Xue, Rui

We have determined column densities of H I and/or H2 for sight lines in the Magellanic Clouds from archival Hubble Space Telescope and Far-Ultraviolet Spectroscopic Explorer spectra of H I Lyα and H2 Lyman-band absorption. Together with some similar data from the literature, we now have absorption-based N(H I) and/or N(H

2012 The Astrophysical Journal
eHST 79