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Supernova Remnant Kes 17: An Efficient Cosmic Ray Accelerator inside a Molecular Cloud
DOI: 10.1088/0004-637X/777/2/148 Bibcode: 2013ApJ...777..148G

Gelfand, Joseph D.; Temim, Tea; Hughes, John P. +3 more

The supernova remnant Kes 17 (SNR G304.6+0.1) is one of a few but growing number of remnants detected across the electromagnetic spectrum. In this paper, we analyze recent radio, X-ray, and γ-ray observations of this object, determining that efficient cosmic ray acceleration is required to explain its broadband non-thermal spectrum. These observat…

2013 The Astrophysical Journal
XMM-Newton 21
Radial profile of the inner heliospheric magnetic field as deduced from Faraday rotation observations
DOI: 10.1051/0004-6361/201220319 Bibcode: 2013A&A...553A.100M

Mancuso, S.; Garzelli, M. V.

Faraday rotation measures (RMs) of the polarized emission from extragalactic radio sources occulted by the coronal plasma were used to infer the radial profile of the inner heliospheric magnetic field near the solar minimum. By inverting LASCO/SOHO polarized brightness (pB) data taken during the observations in May 1997, we retrieved the electron …

2013 Astronomy and Astrophysics
SOHO 21
A Transmission Spectrum of Titan's North Polar Atmosphere from a Specular Reflection of the Sun
DOI: 10.1088/0004-637X/777/2/161 Bibcode: 2013ApJ...777..161B

Nicholson, Philip D.; Sotin, Christophe; Barnes, Jason W. +9 more

Cassini/VIMS T85 observations of a solar specular reflection off of Kivu Lacus (87.°4N 241.°1E) provide an empirical transmission spectrum of Titan's atmosphere. Because this observation was acquired from short range (33,000 km), its intensity makes it visible within the 2.0, 2.7, and 2.8 µm atmospheric windows in addition to the 5 µm …

2013 The Astrophysical Journal
Cassini 21
VLT/XSHOOTER and Subaru/MOIRCS spectroscopy of HUDF.YD3: no evidence for Lyman α emission at z = 8.55
DOI: 10.1093/mnras/stt132 Bibcode: 2013MNRAS.430.3314B

Wilkins, Stephen M.; Bunker, Andrew J.; Caruana, Joseph +5 more

We present spectroscopic observations with VLT/XSHOOTER and Subaru/MOIRCS of a relatively bright Y-band drop-out galaxy in the Hubble Ultra Deep Field (HUDF), first selected by Bunker et al., McLure et al. and Bouwens et al. to be a likely z ≈ 8-9 galaxy on the basis of its colours in the Hubble Space Telescope (HST) Advanced Camera for Surveys an…

2013 Monthly Notices of the Royal Astronomical Society
eHST 21
Herschel Observations of Cataclysmic Variables
DOI: 10.1088/0004-6256/145/1/19 Bibcode: 2013AJ....145...19H

Harrison, Thomas E.; Campbell, Ryan K.; Tappert, Claus +2 more

We have used the PACS instrument on the Herschel Space Observatory to observe eight cataclysmic variables at 70 and 160 µm. Of these eight objects, only AM Her was detected. We have combined the Herschel results with ground-based, Spitzer, and WISE observations to construct spectral energy distributions for all of the targets. For the two dw…

2013 The Astronomical Journal
Herschel 21
Low-frequency Observations of Drifting, Non-thermal Continuum Radio Emission Associated with the Solar Coronal Mass Ejections
DOI: 10.1088/0004-637X/778/1/30 Bibcode: 2013ApJ...778...30R

Ramesh, R.; Kathiravan, C.; Wang, T. J. +3 more

Low-frequency (80 MHz) imaging and spectral (≈85-20 MHz) observations of moving type IV radio bursts associated with coronal mass ejections (CMEs) from the Sun on three different days are reported. The estimated drift speed of the bursts is in the range ≈150-500 km s-1. We find that all three bursts are most likely due to second harmoni…

2013 The Astrophysical Journal
SOHO 21
α Centauri A in the far infrared. First measurement of the temperature minimum of a star other than the Sun
DOI: 10.1051/0004-6361/201220776 Bibcode: 2013A&A...549L...7L

Olofsson, G.; Krivov, A. V.; Eiroa, C. +15 more

Context. Chromospheres and coronae are common phenomena on solar-type stars. Understanding the energy transfer to these heated atmospheric layers requires direct access to the relevant empirical data. Study of these structures has, by and large, been limited to the Sun thus far.
Aims: The region of the temperature reversal can be directly obs…

2013 Astronomy and Astrophysics
Herschel 21
Core electron temperature and density in the innermost Saturn's magnetosphere from HF power spectra analysis on Cassini
DOI: 10.1002/2013JA019199 Bibcode: 2013JGRA..118.7170S

Schippers, P.; Moncuquet, M.; Meyer-Vernet, N. +1 more

We analyze the large-scale structures of electrons in Saturn's inner magnetosphere equatorial plane, from 2.8 to about 10 Saturnian radii (RS). The electron total density and core temperature are obtained using the quasi-thermal noise spectroscopy method, based on the HF power spectra measurements acquired with the Cassini/Radio and Pla…

2013 Journal of Geophysical Research (Space Physics)
Cassini 21
The Herschel-PEP survey: evidence for downsizing in the hosts of dusty star-forming systems
DOI: 10.1093/mnras/stt708 Bibcode: 2013MNRAS.433..127M

Berta, S.; Magnelli, B.; Nordon, R. +27 more

By making use of Herschel PACS Evolutionary Probe observations of the COSMOS and Extended Groth Strip fields, we have estimated the dependence of the clustering properties of FIR-selected sources on their 100 µm fluxes. Our analysis shows a tendency for the clustering strength to decrease with limiting fluxes. By assuming a power-law slope w…

2013 Monthly Notices of the Royal Astronomical Society
Herschel 21
Hubble Space Telescope Imaging of the Binary Nucleus of the Planetary Nebula EGB 6
DOI: 10.1088/0004-637X/769/1/32 Bibcode: 2013ApJ...769...32L

Bond, Howard E.; Gianninas, A.; Ciardullo, Robin +4 more

EGB 6 is an ancient, low-surface-brightness planetary nebula. The central star, also cataloged as PG 0950+139, is a very hot DAOZ white dwarf (WD) with an apparent M dwarf companion, unresolved from the ground but detected initially through excesses in the JHK bands. Its kinematics indicates membership in the Galactic disk population. Inside of EG…

2013 The Astrophysical Journal
eHST 21