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Submillimeter observations of IRAS and WISE debris disk candidates
DOI: 10.1051/0004-6361/201321726 Bibcode: 2013A&A...556A.119B

Dowell, C. D.; De Rosa, R. J.; McCarthy, D. +7 more

A set of six debris disk candidates identified with IRAS or WISE excesses were observed at either 350 µm or 450 µm with the Caltech Submillimeter Observatory. Five of the targets - HIP 51658, HIP 68160, HIP 73512, HIP 76375, and HIP 112460 - have among the largest measured excess emission from cold dust from IRAS in the 25-100 µm…

2013 Astronomy and Astrophysics
Herschel eHST 6
Fluctuations of the intergalactic ionization field at redshift z ~ 2
DOI: 10.1051/0004-6361/201220818 Bibcode: 2013A&A...552A..83A

Reimers, D.; Hagen, H. -J.; Levshakov, S. A. +2 more


Aims: To probe the spectral energy distribution (SED) of the ionizing background radiation at z ≲ 2 and to specify the sources contributing to the intergalactic radiation field.
Methods: The spectrum of a bright quasar HS 1103+6416 (zem = 2.19) contains five successive metal-line absorption systems at z

2013 Astronomy and Astrophysics
eHST 6
The turbulence evolution in the high β region of the Earth's foreshock
DOI: 10.1002/2013JA019424 Bibcode: 2013JGRA..118.7151L

Yuan, Zhigang; Huang, Shiyong; Zhou, Meng +5 more

In this paper, we study the foreshock turbulence evolution in high β region via both Cluster observation on 29 March 2002 and 1-D hybrid simulation. The quasi-sinusoidal and the irregular wave trains are both detected in this event. The former one is believed to be generated by ion-ion right-hand nonresonant instability due to the right-hand polar…

2013 Journal of Geophysical Research (Space Physics)
Cluster 6
Distribution of CO2 in Saturn's Atmosphere from Cassini/cirs Infrared Observations
DOI: 10.1088/0004-637X/776/2/73 Bibcode: 2013ApJ...776...73A

Flasar, F. M.; Achterberg, R. K.; Jennings, D. E. +9 more

This paper focuses on the CO2 distribution in Saturn's atmosphere based on analysis of infrared spectral observations of Saturn made by the Composite Infrared Spectrometer aboard the Cassini spacecraft. The Cassini spacecraft was launched in 1997 October, inserted in Saturn's orbit in 2004 July, and has been successfully making infrared…

2013 The Astrophysical Journal
Cassini 6
Growing evidence for a core formation threshold traced in Herschel Gould Belt survey clouds
DOI: 10.1002/asna.201211956 Bibcode: 2013AN....334..908K

André, Ph.; Arzoumanian, D.; Palmeirim, P. +3 more

It has already been suggested that a threshold in column density - or in visual extinction - may need to be exceeded to form dense cores and then protostars. Based on Herschel Gould Belt survey results in the Aquila and Orion B molecular cloud complexes we observe clear connection between the locations of the detected prestellar cores and their ba…

2013 Astronomische Nachrichten
Herschel 6
WR 138: new results from X-ray and optical spectroscopy
DOI: 10.1051/0004-6361/201322162 Bibcode: 2013A&A...560A..27P

Nazé, Y.; Rauw, G.; De Becker, M. +2 more

Context. Massive-binary evolution models predict that some systems will go through an evolutionary phase where the original primary has become a supernova and left a compact object behind that then orbits a Wolf-Rayet (WR) star. WR 138 is an X-ray bright WR star that has been described as a triple system, including a compact companion in a short-p…

2013 Astronomy and Astrophysics
XMM-Newton 6
Recent Developments in Astrophysical and Cosmological Exploitation of Microwave Surveys
DOI: 10.1142/S0218271813300115 Bibcode: 2013IJMPD..2230011B

Khatri, Rishi; Pointecouteau, Etienne; Toffolatti, Luigi +13 more

In this paper, we focus on the astrophysical results and the related cosmological implications derived from recent microwave surveys, with emphasis to those coming from the Planck mission. We critically discuss the impact of systematic effects and the role of methods to separate the cosmic microwave background (CMB) signal from the astrophysical e…

2013 International Journal of Modern Physics D
XMM-Newton 6
Unexpected Ionization Structure in Eta Carinae's "Weigelt Knots"
DOI: 10.1088/0004-637X/773/1/27 Bibcode: 2013ApJ...773...27R

Davidson, Kris; Mehner, Andrea; Remmen, Grant N.

The Weigelt knots, dense slow-moving ejecta near η Carinae, are mysterious in structure as well as in origin. Using spatially dithered spectrograms obtained with the Hubble Space Telescope/Space Telescope Imaging Spectrograph (HST/STIS), we have partially resolved the ionization zones of one knot. Contrary to simple models, higher ionization level…

2013 The Astrophysical Journal
eHST 6
Aligned grains and inferred toroidal magnetic fields in the envelopes of massive young stellar objects
DOI: 10.1093/mnras/stt1534 Bibcode: 2013MNRAS.435.3419S

Schneider, Glenn; Hines, Dean C.; Wolff, Michael J. +6 more

Massive young stellar objects (YSOs), like low-mass YSOs, are thought to be surrounded by optically thick envelopes and/or discs and are observed to have associated regions that produce polarized light at near-infrared wavelengths. These polarized regions are thought to be lower density outflows along the polar axes of the YSO envelopes. Using the…

2013 Monthly Notices of the Royal Astronomical Society
eHST 6
Statistical Study of 2XMMi-DR3/SDSS-DR8 Cross-correlation Sample
DOI: 10.1088/0004-6256/145/2/42 Bibcode: 2013AJ....145...42Z

Zhao, Yong-Heng; Wu, Xue-Bing; Zhou, Xin-Lin +1 more

Cross-correlating the XMM-Newton 2XMMi-DR3 catalog with the Sloan Digital Sky Survey (SDSS) Data Release 8, we obtain one of the largest X-ray/optical catalogs and explore the distribution of various classes of X-ray emitters in the multidimensional photometric parameter space. Quasars and galaxies occupy different zones while stars scatter in the…

2013 The Astronomical Journal
XMM-Newton 6