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V838 Monocerotis: the central star and its environment a decade after outburst
DOI: 10.1051/0004-6361/201424458 Bibcode: 2014A&A...569L...3C

Meilland, A.; Millour, F.; Chesneau, O. +8 more


Aims: V838 Monocerotis erupted in 2002, brightened in a series of outbursts, and eventually developed a spectacular light echo. A very red star emerged a few months after the outburst. The whole event has been interpreted as the result of a merger.
Methods: We obtained near- and mid-IR interferometric observations of V838 Mon

2014 Astronomy and Astrophysics
AKARI 32
Principal component analysis of MCG-06-30-15 with XMM-Newton
DOI: 10.1093/mnras/stt1925 Bibcode: 2014MNRAS.437..721P

Fabian, A. C.; Brenneman, L.; Matt, G. +4 more

We analyse the spectral variability of MCG-06-30-15 with 600 k s of XMM-Newton data, including 300 k s of new data from the joint XMM-Newton and NuSTAR 2013 observational campaign. We use principal component analysis to find high-resolution, model-independent spectra of the different variable components of the spectrum. We find that over 99 per ce…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 32
Catalog of short gamma-ray transients detected in the SPI/INTEGRAL experiment
DOI: 10.1134/S106377371405003X Bibcode: 2014AstL...40..235M

Minaev, P. Yu.; Pozanenko, A. S.; Grebenev, S. A. +1 more

We analyzed the data obtained by the SPI telescope onboard the INTEGRAL observatory to search for short transient events with a duration from 1 ms to a few tens of seconds. An algorithm for identifying gamma-ray events against the background of a large number of charged particle interactions with the detector has been developed. The classification…

2014 Astronomy Letters
INTEGRAL 32
Probing the Large and Massive Circumgalactic Medium of a Galaxy at z ~ 0.2 using a Pair of Quasars
DOI: 10.1088/0004-637X/784/1/5 Bibcode: 2014ApJ...784....5M

Muzahid, Sowgat

We present an analysis of two O VI absorbers at redshift z abs = 0.227, which were detected in the spectra of two closely spaced QSO sightlines (Q 0107-025A and B) and observed with the Cosmic Origins Spectrograph onboard the Hubble Space Telescope. At the same redshift, the presence of a single bright (~1.2L sstarf) galaxy a…

2014 The Astrophysical Journal
eHST 32
Outflows from active galactic nuclei: the BLR-NLR metallicity correlation
DOI: 10.1093/mnras/stt2386 Bibcode: 2014MNRAS.438.2828D

Valls-Gabaud, David; Du, Pu; Hu, Chen +4 more

The metallicity of active galactic nuclei (AGNs), which can be measured by emission line ratios in their broad- and narrow-line regions (BLRs and NLRs), provides invaluable information about the physical connection between the different components of AGNs. From the archival data bases of the International Ultraviolet Explorer, the Hubble Space Tel…

2014 Monthly Notices of the Royal Astronomical Society
IUE eHST 32
Orbital apocenter is not a sufficient condition for HST/STIS detection of Europa's water vapor aurora
DOI: 10.1073/pnas.1416671111 Bibcode: 2014PNAS..111E5123R

Nimmo, Francis; Saur, Joachim; Roth, Lorenz +4 more

We report far-ultraviolet observations of Jupiter's moon Europa taken by Space Telescope Imaging Spectrograph (STIS) of the Hubble Space Telescope (HST) in January and February 2014 to test the hypothesis that the discovery of a water vapor aurora in December 2012 by local hydrogen (H) and oxygen (O) emissions with the STIS originated from plume a…

2014 Proceedings of the National Academy of Science
eHST 32
Herschel celestial calibration sources. Four large main-belt asteroids as prime flux calibrators for the far-IR/sub-mm range
DOI: 10.1007/s10686-013-9357-y Bibcode: 2014ExA....37..253M

Pearson, Chris; Lim, Tanya; Linz, Hendrik +9 more

Celestial standards play a major role in observational astrophysics. They are needed to characterise the performance of instruments and are paramount for photometric calibration. During the Herschel Calibration Asteroid Preparatory Programme approximately 50 asteroids have been established as far-IR/sub-mm/mm calibrators for Herschel. The selected…

2014 Experimental Astronomy
Herschel 32
HESS J1640-465 - an exceptionally luminous TeV γ-ray supernova remnant
DOI: 10.1093/mnras/stu139 Bibcode: 2014MNRAS.439.2828A

Klochkov, D.; Santangelo, A.; Quirrenbach, A. +217 more

The results of follow-up observations of the TeV γ-ray source HESS J1640-465 from 2004 to 2011 with the High Energy Stereoscopic System (HESS) are reported in this work. The spectrum is well described by an exponential cut-off power law with photon index Γ = 2.11 ± 0.09stat ± 0.10sys, and a cut-off energy of E_c = 6.0^{+2.0}_…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 32
Constraining topological defects with temperature and polarization anisotropies
DOI: 10.1103/PhysRevD.90.103504 Bibcode: 2014PhRvD..90j3504L

Kunz, Martin; Liddle, Andrew R.; Lizarraga, Joanes +3 more

We analyze the possible contribution of topological defects to cosmic microwave anisotropies, both temperature and polarization. We allow for the presence of both inflationary scalars and tensors, and of polarized dust foregrounds that may contribute to or dominate the B-mode polarization signal. We confirm and quantify our previous statements tha…

2014 Physical Review D
Planck 32
Interferometric Follow-up of WISE Hyper-luminous Hot, Dust-obscured Galaxies
DOI: 10.1088/0004-637X/793/1/8 Bibcode: 2014ApJ...793....8W

Tsai, Chao-Wei; Gelino, Christopher R.; Wright, Edward L. +10 more

The Wide-field Infrared Survey Explorer (WISE) has discovered an extraordinary population of hyper-luminous dusty galaxies that are faint in the two bluer passbands (3.4 µm and 4.6 µm) but are bright in the two redder passbands of WISE (12 µm and 22 µm). We report on initial follow-up observations of three of these hot, dus…

2014 The Astrophysical Journal
eHST 32