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Coronal mass ejections—Propagation time and associated internal energy
DOI: 10.1016/j.jastp.2011.01.017 Bibcode: 2011JASTP..73..671M

Mujiber Rahman, A.; Manoharan, P. K.

In this paper, we analyze 91 coronal mass ejection (CME) events studied by Manoharan et al. (2004) and Gopalswamy and Xie (2008). These earth-directed CMEs are large (width >160) and cover a wide range of speeds (∼120-2400kms-1) in the LASCO field of view. This set of events also includes interacting CMEs and some of them…

2011 Journal of Atmospheric and Solar-Terrestrial Physics
SOHO 30
Suzaku View of the Supernova Remnant RCW 86: X-Ray Studies of Newly-Discovered Fe-Rich Ejecta
DOI: 10.1093/pasj/63.sp3.S837 Bibcode: 2011PASJ...63S.837Y

Yamaguchi, Hiroya; Koyama, Katsuji; Uchida, Hiroyuki

We report on results of imaging and spectral analysis of the supernova remnant (SNR) RCW 86 observed with Suzaku. The SNR is known to exhibit K-shell emission of low ionized Fe, possibly originating from supernova ejecta. We revealed the global distribution of the Fe-rich plasma in the entire remnant, for the first time; the Fe-K emission was clea…

2011 Publications of the Astronomical Society of Japan
Suzaku 30
The red supergiants and Wolf-Rayet stars of NGC 604
DOI: 10.1111/j.1365-2966.2010.17676.x Bibcode: 2011MNRAS.411..235E

Relaño, Mónica; Eldridge, John J.

We study the post-main-sequence stars in NGC 604, the most luminous H II region in M33. A number of Wolf-Rayet (WR) stars and one red supergiant (RSG) were discovered earlier. Based on the broad-band photometry of the region, we present evidence that is consistent with the presence of this RSG and with three more RSG candidates. Using spectral ene…

2011 Monthly Notices of the Royal Astronomical Society
eHST 30
Goldschmidt crater and the Moon's north polar region: Results from the Moon Mineralogy Mapper (M3)
DOI: 10.1029/2010JE003702 Bibcode: 2011JGRE..116.0G02C

Clark, R. N.; Head, J. W.; McCord, T. B. +10 more

Soils within the impact crater Goldschmidt have been identified as spectrally distinct from the local highland material. High spatial and spectral resolution data from the Moon Mineralogy Mapper (M3) on the Chandrayaan-1 orbiter are used to examine the character of Goldschmidt crater in detail. Spectral parameters applied to a north pol…

2011 Journal of Geophysical Research (Planets)
Chandrayaan-1 30
Modeling of the HerMES Submillimeter Source Lensed by a Dark Matter Dominated Foreground Group of Galaxies
DOI: 10.1088/0004-637X/738/2/125 Bibcode: 2011ApJ...738..125G

Pérez-Fournon, I.; Rodighiero, G.; Valtchanov, I. +85 more

We present the results of a gravitational lensing analysis of the bright z s = 2.957 submillimeter galaxy (SMG) HERMES found in the Herschel/SPIRE science demonstration phase data from the Herschel Multi-tiered Extragalactic Survey (HerMES) project. The high-resolution imaging available in optical and near-IR channels, along with CO emi…

2011 The Astrophysical Journal
Herschel 30
A Statistical Model for the γ-ray Variability of the Crab Nebula
DOI: 10.1088/2041-8205/730/2/L15 Bibcode: 2011ApJ...730L..15Y

Yuan, Qiang; Zhang, Bing; Wu, Xue-Feng +3 more

A statistical scenario is proposed to explain the γ-ray variability and flares of the Crab Nebula, which were observed recently by the Fermi/LAT. In this scenario electrons are accelerated in a series of knots, whose sizes follow a power-law distribution. These knots presumably move outward from the pulsar and have a distribution in the Doppler bo…

2011 The Astrophysical Journal
INTEGRAL 30
Violent interaction between the active galactic nucleus and the hot gas in the core of the galaxy cluster Sérsic 159-03
DOI: 10.1111/j.1365-2966.2011.18957.x Bibcode: 2011MNRAS.415.3369W

Simionescu, A.; Sun, M.; Allen, S. W. +7 more

We present a multiwavelength study of the energetic interaction between the central active galactic nucleus (AGN), the intracluster medium (ICM) and the optical emission-line nebula in the galaxy cluster Sérsic 159-03. We use X-ray data from Chandra, high-resolution X-ray spectra and ultraviolet (UV) images from XMM-Newton, Hα images from the Sout…

2011 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 30
Benchmarking atomic data for astrophysics: Fe xiii EUV lines
DOI: 10.1051/0004-6361/201117121 Bibcode: 2011A&A...533A..12D

Del Zanna, G.

Recent atomic data for Fe xiii are benchmarked against high-resolution spectroscopic observations of the solar corona. All the identifications of the EUV lines are reviewed by also taking into account laboratory measurements. A few new identifications are proposed, and many wavelengths are revised. All the strongest EUV lines are now identified. V…

2011 Astronomy and Astrophysics
Hinode 30
Evidence of volcanic and glacial activity in Chryse and Acidalia Planitiae, Mars
DOI: 10.1016/j.icarus.2011.01.004 Bibcode: 2011Icar..212..597M

Mellon, Michael T.; McEwen, Alfred S.; Keszthelyi, Laszlo P. +3 more

Chryse and Acidalia Planitiae show numerous examples of enigmatic landforms previously interpreted to have been influenced by a water/ice-rich geologic history. These landforms include giant polygons bounded by kilometer-scale arcuate troughs, bright pitted mounds, and mesa-like features. To investigate the significance of the last we have analyze…

2011 Icarus
MEx 30
The brightness of magnetic field concentrations in the quiet Sun
DOI: 10.1051/0004-6361/201015976 Bibcode: 2011A&A...532A.136S

Schnerr, R. S.; Spruit, H. C.

In addition to the "facular" brightening of active regions, the quiet Sun also contains a small scale magnetic field with associated brightenings in continuum radiation. We measure this contribution of quiet regions to the Sun's brightness from high spatial resolution (0.16 arcsec-0.32 arcsec) observations of the Swedish 1-m Solar Telescope (SST) …

2011 Astronomy and Astrophysics
Hinode 30