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A State Transition of the Luminous X-Ray Binary in the Low-metallicity Blue Compact Dwarf Galaxy I Zw 18
DOI: 10.1088/0004-637X/770/1/20 Bibcode: 2013ApJ...770...20K

Feng, Hua; Kaaret, Philip

We present a measurement of the X-ray spectrum of the luminous X-ray binary in I Zw 18, the blue compact dwarf galaxy with the lowest known metallicity. We find the highest flux yet observed, corresponding to an intrinsic luminosity near 1 × 1040 erg s-1 establishing it as an ultraluminous X-ray source (ULX). The energy spect…

2013 The Astrophysical Journal
XMM-Newton 23
SHARDS: stellar populations and star formation histories of a mass-selected sample of 0.65 < z < 1.1 galaxies
DOI: 10.1093/mnras/stt1165 Bibcode: 2013MNRAS.434.2136H

Barro, Guillermo; Pérez-González, Pablo G.; Tresse, Laurence +10 more

We report on results from the analysis of a stellar mass-selected (log (M*/M) ≥ 9.0) sample of 1644 galaxies at 0.65 < z < 1.1 with ultradeep (mAB < 26.5) optical medium-band (R ∼ 50) photometry from the Survey for High-z Absorption Red and Dead Sources (SHARDS). The spectral resolution of SHARDS allows u…

2013 Monthly Notices of the Royal Astronomical Society
eHST 23
Rapid loss of the plasma sheet energetic electrons associated with the growth of whistler mode waves inside the bursty bulk flows
DOI: 10.1002/2013JA019109 Bibcode: 2013JGRA..118.7200L

Cao, J. B.; Yang, J. Y.; Yu, J. +5 more

the interval ~07:45:36-07:54:24 UT on 24 August 2005, Cluster satellites (C1 and C3) observed an obvious loss of energetic electrons (~3.2-95 keV) associated with the growth of whistler mode waves inside some bursty bulk flows (BBFs) in the midtail plasma sheet (XGSM ~ -17.25 RE). However, the fluxes of the higher-energy elec…

2013 Journal of Geophysical Research (Space Physics)
Cluster 23
Direct Detections of Young Stars in Nearby Elliptical Galaxies
DOI: 10.1088/0004-637X/770/2/137 Bibcode: 2013ApJ...770..137F

Bregman, Joel N.; Ford, H. Alyson

Small amounts of star formation in elliptical galaxies are suggested by several results: surprisingly young ages from optical line indices, cooling X-ray gas, and mid-infrared dust emission. Such star formation has previously been difficult to directly detect, but using ultraviolet Hubble Space Telescope Wide Field Camera 3 imaging, we have identi…

2013 The Astrophysical Journal
eHST 23
Sunskirting comets discovered with the LASCO coronagraphs over the decade 1996-2008
DOI: 10.1016/j.icarus.2013.07.035 Bibcode: 2013Icar..226.1350L

Llebaria, A.; Lamy, P.; A'Hearn, M. F. +3 more

In addition to an unprecedented number of Kreutz sungrazing comets, the LASCO coronagraphs have discovered some 238 unrelated “sunskirting” comets over the 12 years from 1996 to 2008. This new class is organized in several groups, and at least two comets have further been found periodic. This article presents the photometry and the heliocentric li…

2013 Icarus
SOHO 23
Multiscale Magnetic Underdense Regions on the Solar Surface: Granular and Mesogranular Scales
DOI: 10.1007/s11207-012-0179-2 Bibcode: 2013SoPh..282..379B

Giordano, S.; Berrilli, F.; Scardigli, S.

The Sun is a non-equilibrium, dissipative system subject to an energy flow that originates in its core. Convective overshooting motions create temperature and velocity structures that show a temporal and spatial multiscale evolution. As a result, photospheric structures are generally considered to be a direct manifestation of convective plasma mot…

2013 Solar Physics
Hinode 23
Water Maser Survey on AKARI and IRAS Sources: A Search for "Low-velocity" Water Fountains
DOI: 10.1088/0004-637X/769/1/20 Bibcode: 2013ApJ...769...20Y

Kwok, Sun; Yung, Bosco H. K.; Nakashima, Jun-ichi +3 more

We present the results of a 22 GHz H2O maser survey toward a new sample of asymptotic giant branch (AGB) and post-AGB star candidates. Most of the objects are selected for the first time based on the AKARI data, which have high flux sensitivity in the mid-infrared ranges. We aim at finding H2O maser sources in the transient p…

2013 The Astrophysical Journal
AKARI 23
Quasi-periodic oscillations and energy spectra from the two brightest Ultra-Luminous X-ray sources in M82
DOI: 10.1093/mnras/stt1807 Bibcode: 2013MNRAS.436.3262C

Belloni, T.; Zampieri, L.; Caballero-García, M. D.

Ultra-Luminous X-ray sources (ULXs) are thought to be accreting black holes (BHs) that might host intermediate-mass black holes (IMBH), proposed to exist by theoretical studies, even though a firm detection (as a class) is still missing. The brightest ULX in M82 (M82 X-1) is probably one of the best candidates to host an IMBH. In this work, we ana…

2013 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23
Deep hard X-ray survey of the Large Magellanic Cloud
DOI: 10.1093/mnras/sts008 Bibcode: 2013MNRAS.428...50G

Tsygankov, S. S.; Lutovinov, A. A.; Grebenev, S. A. +1 more

Results of the deep survey of the Large Magellanic Cloud (LMC) obtained with the INTEGRAL observatory are presented. The long exposure ( ∼ 7 Ms) allowed us to detect 21 sources in this sky region: ten belonging to the LMC itself (7 HMXBs, 2 PSRs, 1 LMXB), six of extragalactic origin and three belonging to other galaxies in the Local Group - the Mi…

2013 Monthly Notices of the Royal Astronomical Society
INTEGRAL 23
Dependence of O+ escape rate from the Venusian upper atmosphere on IMF directions
DOI: 10.1002/grl.50392 Bibcode: 2013GeoRL..40.1682M

Fedorov, A.; Barabash, S.; Futaana, Y. +5 more

investigate the dependence of the O+ escape rate on the upstream interplanetary magnetic field (IMF) direction by using data from the Analyser of Space Plasma and Energetic Atoms (ASPERA-4) instrument and the magnetometer (MAG) onboard Venus Express. We consider two cases, namely the perpendicular IMF case (167 events) and the parallel …

2013 Geophysical Research Letters
VenusExpress 23