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NuSTAR Discovery of an Unusually Steady Long-term Spin-up of the Be Binary 2RXP J130159.6-635806
DOI: 10.1088/0004-637X/809/2/140 Bibcode: 2015ApJ...809..140K

Hailey, Charles J.; Chakrabarty, Deepto; Fürst, Felix +14 more

We present spectral and timing analyses of Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the accreting X-ray pulsar 2RXP J130159.6-635806. The source was serendipitously observed during a campaign focused on the gamma-ray binary PSR B1259-63 and was later targeted for a dedicated observation. The spectrum has a typical shape for a…

2015 The Astrophysical Journal
XMM-Newton 17
Systematic characterization of the Herschel SPIRE Fourier Transform Spectrometer
DOI: 10.1093/mnras/stv353 Bibcode: 2015MNRAS.449.2274H

Valtchanov, I.; Clements, D. L.; Spencer, L. D. +17 more

A systematic programme of calibration observations was carried out to monitor the performance of the Spectral and Photometric Imaging REceiver (SPIRE) Fourier Transform Spectrometer (FTS) instrument on board the Herschel Space Observatory. Observations of planets (including the prime point-source calibrator, Uranus), asteroids, line sources, dark …

2015 Monthly Notices of the Royal Astronomical Society
Herschel 17
Properties and nature of Be stars. 30. Reliable physical properties of a semi-detached B9.5e+G8III binary BR CMi = HD 61273 compared to those of other well studied semi-detached emission-line binaries
DOI: 10.1051/0004-6361/201424640 Bibcode: 2015A&A...573A.107H

Wolf, M.; Frémat, Y.; Royer, F. +13 more

Reliable determination of the basic physical properties of hot emission-line binaries with Roche-lobe filling secondaries is important for developing the theory of mass exchange in binaries. It is a very hard task, however, which is complicated by the presence of circumstellar matter in these systems. So far, only a small number of systems with ac…

2015 Astronomy and Astrophysics
Hipparcos 16
Fossil group origins - VI. Global X-ray scaling relations of fossil galaxy clusters
DOI: 10.1093/mnras/stv1879 Bibcode: 2015MNRAS.454..161K

De Grandi, S.; Gastaldello, F.; Jiménez-Bailón, E. +11 more

We present the first pointed X-ray observations of 10 candidate fossil galaxy groups and clusters. With these Suzaku observations, we determine global temperatures and bolometric X-ray luminosities of the intracluster medium (ICM) out to r500 for six systems in our sample. The remaining four systems show signs of significant contaminati…

2015 Monthly Notices of the Royal Astronomical Society
Suzaku 16
Carbon, Helium, and Proton Kinetic Temperatures in a Cygnus Loop Shock Wave
DOI: 10.1088/0004-637X/805/2/152 Bibcode: 2015ApJ...805..152R

Blair, William P.; Raymond, John C.; Ghavamian, Parviz +1 more

Observations of SN 1006 have shown that ions and electrons in the plasma behind fast supernova remnant shock waves are far from equilibrium, with the electron temperature much lower than the proton temperature and ion temperatures approximately proportional to ion mass. In the ∼360 km s-1shock waves of the Cygnus Loop, on the other hand…

2015 The Astrophysical Journal
eHST 16
Episodes of fluvial and volcanic activity in Mangala Valles, Mars
DOI: 10.1016/j.icarus.2014.09.040 Bibcode: 2015Icar..245..333K

Daubar, Ingrid J.; McEwen, Alfred S.; Hamilton, Christopher W. +1 more

A new mapping-based study of the 900-km-long Mangala Valles outflow system was motivated by the availability of new high-resolution images and continued debates about the roles of water and lava in outflow channels on Mars. This study uses photogeologic analysis, geomorphic surface mapping, cratering statistics, and relative stratigraphy. Results …

2015 Icarus
MEx 16
Channel slope reversal near the Martian dichotomy boundary: Testing tectonic hypotheses
DOI: 10.1016/j.geomorph.2014.09.028 Bibcode: 2015Geomo.240..121L

Nimmo, Francis; Burr, Devon M.; Jacobsen, Robert E. +1 more

Faults along the Martian dichotomy boundary are evidence of tectonic activity, which by analogy with terrestrial tectonism may cause changes in or even reversal of fluvial longitudinal profiles. In the eastern hemisphere between 30° E and 150° E, this tectonic activity has been hypothesized to result from lower crustal flow or from lithospheric fl…

2015 Geomorphology
MEx 16
Cassini VIMS observations of H3+ emission on the nightside of Jupiter
DOI: 10.1002/2015JA021097 Bibcode: 2015JGRA..120.6948S

Baines, Kevin H.; Brown, Robert H.; O'Donoghue, James +10 more

We present the first detailed analysis of H3+ nightside emission from Jupiter, using Visual and Infrared Mapping Spectrometer (VIMS) data from the Cassini flyby in 2000-2001, producing the first Jovian maps of nightside H3+ emission, temperature, and column density. Using these, we identify and character…

2015 Journal of Geophysical Research (Space Physics)
Cassini 16
The SWIFT AGN and Cluster Survey. I. Number Counts of AGNs and Galaxy Clusters
DOI: 10.1088/0067-0049/218/1/8 Bibcode: 2015ApJS..218....8D

Bregman, Joel N.; Kochanek, Christopher S.; Dai, Xinyu +2 more

The Swift active galactic nucleus (AGN) and Cluster Survey (SACS) uses 125 deg2 of Swift X-ray Telescope serendipitous fields with variable depths surrounding γ-ray bursts to provide a medium depth (4× {{10}-15} erg cm-2 s-1) and area survey filling the gap between deep, narrow Chandra/XMM-Newton surveys…

2015 The Astrophysical Journal Supplement Series
Planck 16
A Suzaku view of IGR J16393-4643
DOI: 10.1093/mnras/stu2395 Bibcode: 2015MNRAS.446.4148I

Maitra, Chandreyee; Paul, Biswajit; Pradhan, Pragati +1 more

The pulsar IGR J16393-4643 belongs to a class of highly absorbed supergiant high-mass X-ray binaries (HMXBs), characterized by a very high column density of absorbing matter. We present the results of simultaneous broad-band pulsation and spectrum analysis from a 44-ks Suzaku observation of the source. The orbital intensity profile created with th…

2015 Monthly Notices of the Royal Astronomical Society
Suzaku 16