Search Publications

New results and questions of lunar exploration from SELENE, Chang'E-1, Chandrayaan-1 and LRO/LCROSS
DOI: 10.1016/j.asr.2012.11.022 Bibcode: 2013AdSpR..52..285J

Jin, Shuanggen; Arivazhagan, Sundaram; Araki, Hiroshi

The moon has longstanding questions such as lunar environments, origin, formation and evolution, magnetization of crustal rocks, internal structure and possible life. The recent lunar missions, e.g., SELenological and ENgineering Explorer "KAGUYA" (SELENE), Chang'E-1, Chandrayaan-1, and Lunar Reconnaissance Orbiter/Lunar CRater Observation and Sen…

2013 Advances in Space Research
Chandrayaan-1 35
A bright ultraluminous X-ray source in NGC 5907
DOI: 10.1093/mnras/stt1133 Bibcode: 2013MNRAS.434.1702S

Sutton, Andrew D.; Roberts, Timothy P.; Goad, Michael R. +4 more

We present a multimission X-ray analysis of a bright (peak observed 0.3-10 keV luminosity of ∼6 × 1040 erg s-1), but relatively highly absorbed ultraluminous X-ray source (ULX) in the edge-on spiral galaxy NGC 5907. The ULX is spectrally hard in X-rays (Γ ∼ 1.2-1.7, when fitted with an absorbed power law), and has a previousl…

2013 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 35
Chandra View of the Warm-hot Intergalactic Medium toward 1ES 1553+113: Absorption-line Detections and Identifications. I.
DOI: 10.1088/0004-637X/769/2/90 Bibcode: 2013ApJ...769...90N

Piro, L.; Shull, J. M.; Barcons, X. +14 more

We present the first results from our pilot 500 ks Chandra Low Energy Transmission Grating Large Program observation of the soft X-ray brightest source in the z >~ 0.4 sky, the blazar 1ES 1553+113, aimed to secure the first uncontroversial detections of the missing baryons in the X-rays. We identify a total of 11 possible absorption lines, with…

2013 The Astrophysical Journal
eHST 35
Multiple stellar populations in Magellanic Cloud clusters. II. Evidence also in the young NGC 1844?
DOI: 10.1051/0004-6361/201220567 Bibcode: 2013A&A...555A.143M

Anderson, J.; Milone, A. P.; Bedin, L. R. +4 more

We used Hubble Space Telescope observations to study the young cluster NGC 1844 in the Large Magellanic Cloud (LMC). We estimated the fraction and the mass-ratio distribution of photometric binaries and report that the main sequence presents an intrinsic breadth which cannot be explained only in terms of photometric errors, and is unlikely because…

2013 Astronomy and Astrophysics
eHST 35
Phobos 2/ASPERA data revisited: Planetary ion escape rate from Mars near the 1989 solar maximum
DOI: 10.1002/grl.50149 Bibcode: 2013GeoRL..40..477R

Barabash, Stas; Lundin, Rickard; Nilsson, Hans +4 more

Insights about the near-Mars space environment from Mars Express observations have motivated a revisit of the Phobos 2/ASPERA ion data from 1989. We have expanded the analysis to now include all usable heavy ion (O+, O2+, CO2+) measurements from the circular orbits of Phobos 2. Phobos 2/ASPERA ion fluxes in the Martian tail are compared…

2013 Geophysical Research Letters
MEx 35
On the chemical composition of Titan’s dry lakebed evaporites
DOI: 10.1016/j.icarus.2013.07.026 Bibcode: 2013Icar..226.1431C

Barnes, J. W.; Cordier, D.; Ferreira, A. G.

Titan, the main satellite of Saturn, has an active cycle of methane in its troposphere. Among other evidence for a mechanism of evaporation at work on the ground, dry lakebeds have been discovered. Recent Cassini infrared observations of these empty lakes have revealed a surface composition poor in water ice compared to that of the surrounding ter…

2013 Icarus
Cassini 35
Multiwavelength campaign on Mrk 509. XI. Reverberation of the Fe Kα line
DOI: 10.1051/0004-6361/201219450 Bibcode: 2013A&A...549A..72P

Kaastra, J. S.; Kriss, G. A.; Arav, N. +17 more

Context. We report on a detailed study of the Fe K emission/absorption complex in the nearby, bright Seyfert 1 galaxy Mrk 509. The study is part of an extensive XMM-Newton monitoring consisting of 10 pointings (~60 ks each) about once every 4 days, and includes a reanalysis of previous XMM-Newton and Chandra observations.
Aims: We aim at unde…

2013 Astronomy and Astrophysics
XMM-Newton 34
The Exceptional Soft X-Ray Halo of the Galaxy Merger NGC 6240
DOI: 10.1088/0004-637X/765/2/141 Bibcode: 2013ApJ...765..141N

Zezas, A.; Elvis, M.; Pellegrini, S. +5 more

We report on a recent ~150 ks long Chandra observation of the ultraluminous infrared galaxy merger NGC 6240, which allows a detailed investigation of the diffuse galactic halo. Extended soft X-ray emission is detected at the 3σ confidence level over a diamond-shaped region with projected physical size of ~110 × 80 kpc, and a single-component therm…

2013 The Astrophysical Journal
eHST 34
Nonlinear Force-free Magnetic Field Fitting to Coronal Loops with and without Stereoscopy
DOI: 10.1088/0004-637X/763/2/115 Bibcode: 2013ApJ...763..115A

Aschwanden, Markus J.

We developed a new nonlinear force-free magnetic field (NLFFF) forward-fitting algorithm based on an analytical approximation of force-free and divergence-free NLFFF solutions, which requires as input a line-of-sight magnetogram and traced two-dimensional (2D) loop coordinates of coronal loops only, in contrast to stereoscopically triangulated thr…

2013 The Astrophysical Journal
SOHO 34
Determination of an Upper Limit for the Water Outgassing Rate of Main-belt Comet P/2012 T1 (PANSTARRS)
DOI: 10.1088/2041-8205/774/1/L13 Bibcode: 2013ApJ...774L..13O

Hartogh, P.; Teyssier, D.; Biver, N. +8 more

A new Main-Belt Comet (MBC) P/2012 T1 (PANSTARRS) was discovered on 2012 October 6, approximately one month after its perihelion, by the Pan-STARRS1 survey based in Hawaii. It displayed cometary activity upon its discovery with one hypothesis being that the activity was driven by sublimation of ices; as a result, we searched for emission assumed t…

2013 The Astrophysical Journal
Herschel 34