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A multiwavelength infrared study of NGC 891
DOI: 10.1111/j.1365-2966.2009.14532.x Bibcode: 2009MNRAS.395...97W

Madden, S. C.; Galliano, F.; Bendo, G. J. +2 more

We present a multiwavlength infrared (IR) study of the nearby, edge-on, spiral galaxy NGC 891. We have examined 20 independent, spatially resolved IR images of this galaxy, 14 of which are newly reduced and/or previously unpublished images. These images span a wavelength regime from λ1.2µm in which the emission is dominated by cool stars, th…

2009 Monthly Notices of the Royal Astronomical Society
ISO 30
A Smoking Gun in the Carina Nebula
DOI: 10.1088/0004-637X/695/1/L4 Bibcode: 2009ApJ...695L...4H

Hamaguchi, Kenji; Corcoran, Michael F.; Petre, Rob +8 more

The Carina Nebula is one of the youngest, most active sites of massive star formation in our Galaxy. In this nebula, we have discovered a bright X-ray source that has persisted for ~30 years. The soft X-ray spectrum, consistent with kT ~ 128 eV blackbody radiation with mild extinction, and no counterpart in the near- and mid-infrared wavelengths i…

2009 The Astrophysical Journal
XMM-Newton 30
Evidence for Morphology and Luminosity Transformation of Galaxies at High Redshifts
DOI: 10.1088/0004-637X/700/1/791 Bibcode: 2009ApJ...700..791H

Hwang, Ho Seong; Park, Changbom

We study the galaxy morphology-luminosity-environmental relation and its redshift evolution using a spectroscopic sample of galaxies in the Great Observatories Origins Deep Survey. In the redshift range of 0.4 <= z <= 1.0, we detect conformity in morphology between neighboring galaxies. The realm of conformity is confined within the virializ…

2009 The Astrophysical Journal
eHST 30
Young stars and protostellar cores near NGC 2023
DOI: 10.1051/0004-6361/200912550 Bibcode: 2009A&A...507.1485M

Mookerjea, B.; Sandell, G.; Jarrett, T. H. +1 more

Context: We investigate the young (proto)stellar population in NGC 2023 and the L 1630 molecular cloud bordering the h ii region IC 434, using Spitzer IRAC and MIPS archive data, JCMT SCUBA imaging and spectroscopy as well as targeted BIMA observations of one of the Class 0 protostars, NGC 2023 MM 1.
Aims: We study the distribution of gas, dus…

2009 Astronomy and Astrophysics
IUE XMM-Newton 30
A Very Large Array Radio Survey of Early-Type Galaxies in the Virgo Cluster
DOI: 10.1088/0004-6256/138/6/1990 Bibcode: 2009AJ....138.1990C

Axon, David J.; Merritt, David; Capetti, Alessandro +2 more

We present the results of an 8.4 GHz Very Large Array radio survey of early-type galaxies extracted from the sample selected by Côté and collaborators for the Advanced Camera for Surveys Virgo Cluster Survey. The aim of this survey is to investigate the origin of radio emission in early-type galaxies and its link with the host properties in an une…

2009 The Astronomical Journal
eHST 30
On the origin of the 511-keV emission in the Galactic Centre
DOI: 10.1111/j.1365-2966.2008.14113.x Bibcode: 2009MNRAS.392.1115B

Maccarone, Thomas J.; Taylor, James E.; Silk, Joseph +1 more

Diffuse 511-keV line emission, from the annihilation of cold positrons, has been observed in the direction of the Galactic Centre for more than 30yr. The latest high-resolution maps of this emission produced by the SPI instrument on INTEGRAL suggest at least one component of the emission is spatially coincident with the distribution of ~70 luminou…

2009 Monthly Notices of the Royal Astronomical Society
INTEGRAL 30
Gravity waves in the upper atmosphere of Venus revealed by CO2 nonlocal thermodynamic equilibrium emissions
DOI: 10.1029/2008JE003073 Bibcode: 2009JGRE..114.0B32G

Drossart, P.; Piccioni, G.; Occhipinti, G. +2 more

The imaging capabilities of the Visible and Infrared Thermal Imaging Spectrometer-Mapper (VIRTIS-M) onboard Venus Express mission are used to analyze perturbations of CO2 nonlocal thermodynamic equilibrium emissions in the thermosphere of Venus. These emissions with a wavelength of 4.3 µm originate from the 110-140 km altitude ran…

2009 Journal of Geophysical Research (Planets)
VenusExpress 30
Classification of Extremely Red Objects in the Cosmos Field
DOI: 10.1088/0004-637X/702/2/1458 Bibcode: 2009ApJ...702.1458K

Fang, Guanwen; Kong, Xu; Wang, Min +1 more

We present a study of the classification of z ~ 1 extremely red objects (EROs), using a combination of Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS), Spitzer Infrared Array Camera (IRAC), and ground-based images of the COSMOS field. Our sample includes ~5300 EROs with i - K s >= 2.45 (AB, equivalently I - K s

2009 The Astrophysical Journal
eHST 30
Optical properties of dust from Jupiter family comets
DOI: 10.1016/j.pss.2008.10.015 Bibcode: 2009P&SS...57.1118H

Levasseur-Regourd, A. C.; Hadamcik, E.

To try to define specific physical properties of the dust of Jupiter-family comets (JFCs), we compare the light scattered by them. Amongst the more than 1000 JFCs, less than 200 are numbered, 40 of them being rather bright. In the present work we use data from the latter. In situ observations of three nuclei show low albedo surfaces. The albedo of…

2009 Planetary and Space Science
Giotto 30
Saturn's Magnetospheric Configuration
DOI: 10.1007/978-1-4020-9217-6_9 Bibcode: 2009sfch.book..203G

Persoon, Ann M.; Gombosi, Tamas I.; Krupp, Norbert +5 more

This Chapter summarizes our current understanding of Saturn's magnetospheric configuration. Observations from the Cassini Prime and Equinox Missions have answered some questions and opened new ones. One of the fundamental questions of magnetospheric physics is what are the sources of the plasma that populate the magnetosphere. At Saturn, there is …

2009 Saturn from Cassini-Huygens
Cassini 30