Search Publications

Discovery of new X-ray sources near the unidentified gamma-ray source HESS J1841-055
DOI: 10.1016/j.asr.2015.02.035 Bibcode: 2015AdSpR..55.2493N

Koyama, K.; Nobukawa, M.; Tsuru, T. G. +1 more

HESS J1841-055 is a diffuse unidentified gamma-ray source with the size of ∼1°.3 × 1°. No conclusive counterpart in other wavelengths has so far detected. To search for X-rays responsible for the TeV emission, the Suzaku observations were conducted, which covered a half region of the HESS source. In the soft band (0.5-2.0 keV), we discovered a dif…

2015 Advances in Space Research
Suzaku XMM-Newton 4
Plasma draining and replenishing near a solar active region inferred from cross-correlation between radiation intensity and Doppler shift
DOI: 10.1007/s11430-014-4999-9 Bibcode: 2015ScChD..58..830Z

Wang, Xin; Zhang, JingBo; He, JianSen +3 more

Using observations from the EUV Imaging Spectrometer (EIS) onboard Hinode, we exam the plasma dynamics around the edge of the active region 10977, possibly associated with the source of nascent slow/intermediate solar wind. The correlation between the temporal profiles of the radiation intensity and Doppler shift for each emission line are analyze…

2015 Science China Earth Sciences
Hinode 4
A study on the mid-infrared sources that dramatically brightened
DOI: 10.1093/pasj/psv008 Bibcode: 2015PASJ...67...39O

Matsunaga, Noriyuki; Nakada, Yoshikazu; Ita, Yoshifusa +5 more

We present results of near-infrared (NIR) photometric and spectroscopic observations of mid-infrared (MIR) sources that brightened dramatically. Using Infrared Astronomical Satellite (IRAS), AKARI, and Wide-field Infrared Survey Explorer (WISE) point source catalogs, we found that four sources (IRAS 19574+4941, V2494 Cyg, IRAS 22343+7501, and V583…

2015 Publications of the Astronomical Society of Japan
AKARI 4
SuperModel Analysis of A1246 and J255: On the Evolution of Galaxy Clusters from High to Low Entropy States
DOI: 10.1088/0004-637X/800/1/75 Bibcode: 2015ApJ...800...75F

Lapi, A.; Fusco-Femiano, R.

We present an analysis of high-quality X-ray data out to the virial radius for the two galaxy clusters A1246 and GMBCG J255.34805+64.23661 (J255) by means of our entropy-based SuperModel. For A1246 we find that the spherically averaged entropy profile of the intracluster medium (ICM) progressively flattens outward, and that a nonthermal pressure c…

2015 The Astrophysical Journal
Suzaku 4
The Flybys of Asteroids 2867 Steins, 21 Lutetia, and 4179 Toutatis
DOI: 10.2458/azu_uapress_9780816532131-ch023 Bibcode: 2015aste.book..433B

Barucci, M. A.; Thomas, N.; Fulchignoni, M. +2 more

Three flybys of asteroids have occurred in the period between 2008 and 2012. (2867) Šteins and (21) Lutetia have been observed by the European Space Agency's Rosetta spacecraft, and (4179) Toutatis was observed by the Chinese National Space Agency's Chang'e-2. The properties of these three bodies are very different from other asteroids visited to …

2015 Asteroids IV
Rosetta 4
New Horizons: Long-range Kuiper Belt targets observed by the Hubble Space Telescope
DOI: 10.1016/j.icarus.2014.04.014 Bibcode: 2015Icar..246..369B

Stern, S. A.; Weaver, H. A.; Buie, M. W. +4 more

We report on Hubble Space Telescope (HST) observations of three Kuiper Belt Objects (KBOs), discovered in our dedicated ground-based search campaign, that are candidates for long-range observations from the New Horizons spacecraft: 2011 JY31, 2011 HZ102, and 2013 LU35. Astrometry with HST enables both current and f…

2015 Icarus
eHST 4
Evolution of Kelvin-Helmholtz instability at Venus in the presence of the parallel magnetic field
DOI: 10.1063/1.4922753 Bibcode: 2015PhPl...22f2902L

Zhang, T. L.; Cao, J. B.; Fu, H. S. +2 more

Two-dimensional MHD simulations were performed to study the evolution of the Kelvin-Helmholtz (KH) instability at the Venusian ionopause in response to the strong flow shear in presence of the in-plane magnetic field parallel to the flow direction. The physical behavior of the KH instability as well as the triggering and occurrence conditions for …

2015 Physics of Plasmas
VenusExpress 4
The use of the power density for identifying reconnection regions
DOI: 10.1002/2015JA021535 Bibcode: 2015JGRA..120.8644H

Gunell, H.; Hamrin, M.; Vaivads, A. +2 more

In the vicinity of magnetic reconnection, magnetic energy is transferred into kinetic energy. A reconnection region hence corresponds to a load, and it should manifest itself as large and positive values of the power density, E·J ≫ 0, where E is the electric field and J the current density. In this article we analyze Cluster plasma sheet data from…

2015 Journal of Geophysical Research (Space Physics)
Cluster 4
An obscured narrow-line Seyfert 1 galaxy candidate, Mrk 1388 with nonthermal jets
DOI: 10.1093/pasj/psu147 Bibcode: 2015PASJ...67...15D

Doi, Akihiro

Mrk 1388 has an unusual Seyfert nucleus that shows narrow emission-line components without broad emission-line ones, but shows a strong featureless continuum and strong iron-forbidden, high-ionization emission lines. The apparent coexistence of type-1/2 characteristics is potentially attributed to a heavily obscured broad-line region or to an inte…

2015 Publications of the Astronomical Society of Japan
eHST 4
A Gemini/GMOS Study of Intermediate Luminosity Early-type Virgo Cluster Galaxies. I. Globular Cluster and Stellar Kinematics
DOI: 10.1088/0004-637X/806/1/133 Bibcode: 2015ApJ...806..133L

Jordán, Andrés; Liu, Chengze; Zhang, Hong-xin +10 more

We present a kinematic analysis of the globular cluster (GC) systems and diffuse stellar light of four intermediate luminosity (sub-L*) early-type galaxies in the Virgo cluster based on Gemini Multi-Object Spectrographs (GMOS) data. Our galaxy sample is fainter (-23.8\lt {{M}K}\lt -22.7) than most previous studies, nearly doubling the n…

2015 The Astrophysical Journal
eHST 4