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Can Charge Exchange Explain Anomalous Soft X-Ray Emission in the Cygnus Loop?
DOI: 10.1088/2041-8205/787/2/L31 Bibcode: 2014ApJ...787L..31C

Wu, Y.; Shelton, R. L.; Henley, D. B. +4 more

Recent X-ray studies have shown that supernova shock models are unable to satisfactorily explain X-ray emission in the rim of the Cygnus Loop. In an attempt to account for this "anomalously" enhanced X-ray flux, we fit the region with a model including theoretical charge exchange (CX) data along with shock and background X-ray models. The model in…

2014 The Astrophysical Journal
Suzaku 31
Bridging EUV and White-Light Observations to Inspect the Initiation Phase of a "Two-Stage" Solar Eruptive Event
DOI: 10.1007/s11207-014-0585-8 Bibcode: 2014SoPh..289.4545B

Seaton, D. B.; Habbal, S. R.; Bain, H. M. +2 more

The initiation phase of coronal mass ejections (CMEs) is a very important aspect of solar physics, as these phenomena ultimately drive space weather in the heliosphere. This phase is known to occur between the photosphere and low corona, where many models introduce an instability and/or magnetic reconnection that triggers a CME, often with associa…

2014 Solar Physics
PROBA-2 SOHO 31
A CO Survey in Planet-forming Disks: Characterizing the Gas Content in the Epoch of Planet Formation
DOI: 10.1088/0004-6256/148/3/47 Bibcode: 2014AJ....148...47H

Ménard, F.; Casassus, S.; Eiroa, C. +13 more

We carried out a 12CO(3-2) survey of 52 southern stars with a wide range of IR excesses (L IR/L *) using the single-dish telescopes APEX and ASTE. The main aims were (1) to characterize the evolution of molecular gas in circumstellar disks using L IR/L * values as a proxy of disk dust evolutio…

2014 The Astronomical Journal
IUE 31
Cosmic Ray Transport in Heliospheric Magnetic Structures. I. Modeling Background Solar Wind Using the CRONOS Magnetohydrodynamic Code
DOI: 10.1088/0004-637X/788/1/80 Bibcode: 2014ApJ...788...80W

Fichtner, H.; Heber, B.; Kühl, P. +4 more

The transport of energetic particles such as cosmic rays is governed by the properties of the plasma being traversed. While these properties are rather poorly known for galactic and interstellar plasmas due to the lack of in situ measurements, the heliospheric plasma environment has been probed by spacecraft for decades and provides a unique oppor…

2014 The Astrophysical Journal
SOHO Ulysses 31
Gas Bulk Motion in the Perseus Cluster Measured with Suzaku
DOI: 10.1088/0004-637X/782/1/38 Bibcode: 2014ApJ...782...38T

Fukazawa, Y.; Tamura, T.; Iizuka, R. +8 more

We present the results from Suzaku observations of the Perseus Cluster, which is relatively close, the brightest in the X-ray sky, and a relaxed object with a cool core. A number of exposures of central regions and offset pointing with the X-ray Imaging Spectrometer cover a region within radii of 20'-30'. The central data are used to evaluate the …

2014 The Astrophysical Journal
Suzaku 31
The X-CLASS-redMaPPer galaxy cluster comparison. I. Identification procedures
DOI: 10.1051/0004-6361/201423794 Bibcode: 2014A&A...571A..87S

Pierre, M.; Faccioli, L.; Clerc, N. +5 more

Context. This paper is the first in a series undertaking a comprehensive correlation analysis between optically selected and X-ray-selected cluster catalogues. The rationale of the project is to develop a holistic picture of galaxy clusters utilising optical and X-ray-cluster-selected catalogues with well-understood selection functions.
Aims:…

2014 Astronomy and Astrophysics
XMM-Newton 31
Black hole spin and size of the X-ray-emitting region(s) in the Seyfert 1.5 galaxy ESO 362-G18
DOI: 10.1093/mnras/stu1358 Bibcode: 2014MNRAS.443.2862A

Bianchi, S.; Fabian, A. C.; Miniutti, G. +7 more

We report results from multi-epoch X-ray observations of the Seyfert 1.5 galaxy ESO 362-G18 performed between 2005 November and 2010 June. ESO 362-G18 generally exhibits the typical X-ray spectrum of type 1 active galactic nuclei. A disc-reflection component accounts for broad residuals in the iron K band and above 10 keV, as well as for a signifi…

2014 Monthly Notices of the Royal Astronomical Society
XMM-Newton 31
Probing the solar interface region
DOI: 10.1126/science.346.6207.315 Bibcode: 2014Sci...346..315D

De Pontieu, Bart; Carlsson, Mats; Title, Alan

2014 Science
IRIS 31
Astrometrically Registered Simultaneous Observations of the 22 GHz H2O and 43 GHz SiO Masers toward R Leonis Minoris Using KVN and Source/Frequency Phase Referencing
DOI: 10.1088/0004-6256/148/5/97 Bibcode: 2014AJ....148...97D

Byun, Do-Young; Kim, Jongsoo; Kim, Kee-Tae +22 more

Oxygen-rich asymptotic giant branch (AGB) stars can be intense emitters of SiO (v = 1 and 2, J = 1 → 0) and H2O maser lines at 43 and 22 GHz, respectively. Very long baseline interferometry (VLBI) observations of the maser emission provide a unique tool to probe the innermost layers of the circumstellar envelopes in AGB stars. Neverthel…

2014 The Astronomical Journal
Hipparcos 31
The Secret Lives of Cepheids: Evolutionary Changes and Pulsation-induced Shock Heating in the Prototype Classical Cepheid δ Cep
DOI: 10.1088/0004-637X/794/1/80 Bibcode: 2014ApJ...794...80E

Harper, Graham M.; Guinan, Edward F.; Engle, Scott G. +2 more

Over the past decade, the Secret Lives of Cepheids (SLiC) program has been carried out at Villanova University to study aspects and behaviors of classical Cepheids that are still not well understood. In this, the first of several planned papers on program Cepheids, we report the current results for δ Cep, the Cepheid prototype. Ongoing photometry …

2014 The Astrophysical Journal
IUE XMM-Newton eHST 31