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Plasma Motions and Heating by Magnetic Reconnection in a 2007 May 19 Flare
DOI: 10.1088/0004-637X/741/2/107 Bibcode: 2011ApJ...741..107H

Harra, Louise K.; Hara, Hirohisa; Young, Peter R. +2 more

Based on scanning spectroscopic observations with the Hinode EUV imaging spectrometer, we have found a loop-top hot source, a fast jet nearby, and an inflow structure flowing to the hot source that appeared in the impulsive phase of a long-duration flare at the disk center on 2007 May 19. The hot source observed in Fe XXIII and Fe XXIV emission li…

2011 The Astrophysical Journal
Hinode 88
The Discovery and Nature of the Optical Transient CSS100217:102913+404220
DOI: 10.1088/0004-637X/735/2/106 Bibcode: 2011ApJ...735..106D

Drake, A. J.; Djorgovski, S. G.; Anderson, J. +32 more

We report on the discovery and observations of the extremely luminous optical transient CSS100217:102913+404220 (CSS100217 hereafter). Spectroscopic observations showed that this transient was coincident with a galaxy at redshift z = 0.147 and reached an apparent magnitude of V ~ 16.3. After correcting for foreground Galactic extinction we determi…

2011 The Astrophysical Journal
eHST 88
The Star-formation-rate-Density Relation at 0.6 < z < 0.9 and the Role of Star-forming Galaxies
DOI: 10.1088/0004-637X/735/1/53 Bibcode: 2011ApJ...735...53P

Franx, Marijn; Kelson, Daniel D.; Illingworth, Garth D. +2 more

We study the star formation rates (SFRs) of galaxies as a function of local galaxy density at 0.6 < z < 0.9. We used a low-dispersion prism in IMACS on the 6.5 m Baade (Magellan I) telescope to obtain spectra and measured redshifts to a precision of σ z /(1 + z) ~ 1% for galaxies with z AB < 23.3 mag. We utilized a s…

2011 The Astrophysical Journal
eHST 87
AKARI Observation of the Fluctuation of the Near-infrared Background
DOI: 10.1088/0004-637X/742/2/124 Bibcode: 2011ApJ...742..124M

Lee, H. M.; Jeong, W. -S.; Matsuhara, H. +6 more

We report a search for fluctuations of the sky brightness toward the north ecliptic pole with the Japanese infrared astronomical satellite AKARI, at 2.4, 3.2, and 4.1 µm. We obtained circular maps with 10' diameter fields of view, which clearly show a spatial structure on the scale of a few hundred arcseconds. A power spectrum analysis shows…

2011 The Astrophysical Journal
AKARI 86
Diffuse Emission Measurement with the SPectrometer on INTEGRAL as an Indirect Probe of Cosmic-Ray Electrons and Positrons
DOI: 10.1088/0004-637X/739/1/29 Bibcode: 2011ApJ...739...29B

Jourdain, Elisabeth; Roques, Jean-Pierre; Bouchet, Laurent +3 more

Significant advances have been made in the understanding of the diffuse Galactic hard X-ray continuum emission using data from the INTEGRAL observatory. The diffuse hard power-law component seen with the SPectrometer on INTEGRAL (SPI) has been identified with inverse-Compton emission from relativistic (GeV) electrons on the cosmic microwave backgr…

2011 The Astrophysical Journal
INTEGRAL 85
Molecular Gas in Young Debris Disks
DOI: 10.1088/2041-8205/740/1/L7 Bibcode: 2011ApJ...740L...7M

Apai, D.; Pascucci, I.; Ábrahám, P. +7 more

Gas-rich primordial disks and tenuous gas-poor debris disks are usually considered as two distinct evolutionary phases of the circumstellar matter. Interestingly, the debris disk around the young main-sequence star 49 Ceti possesses a substantial amount of molecular gas and possibly represents the missing link between the two phases. Motivated to …

2011 The Astrophysical Journal
AKARI 85
Observation of High-speed Outflow on Plume-like Structures of the Quiet Sun and Coronal Holes with Solar Dynamics Observatory/Atmospheric Imaging Assembly
DOI: 10.1088/0004-637X/736/2/130 Bibcode: 2011ApJ...736..130T

He, Jiansen; Habbal, Shadia Rifai; McIntosh, Scott W. +1 more

Observations from the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory reveal ubiquitous episodic outflows (jets) with an average speed around 120 km s-1 at temperatures often exceeding a million degree in plume-like structures, rooted in magnetized regions of the quiet solar atmosphere. These outflows are not restric…

2011 The Astrophysical Journal
Hinode 85
A Combined Low-radio Frequency/X-ray Study of Galaxy Groups. I. Giant Metrewave Radio Telescope Observations at 235 MHz AND 610 MHz
DOI: 10.1088/0004-637X/732/2/95 Bibcode: 2011ApJ...732...95G

Raychaudhury, Somak; Jones, Christine; Clarke, Tracy E. +12 more

We present new Giant Metrewave Radio Telescope observations at 235 MHz and 610 MHz of 18 X-ray bright galaxy groups. These observations are part of an extended project, presented here and in future papers, which combines low-frequency radio and X-ray data to investigate the interaction between central active galactic nuclei (AGNs) and the intra-gr…

2011 The Astrophysical Journal
XMM-Newton 84
A Comparative Study of Confined and Eruptive Flares in NOAA AR 10720
DOI: 10.1088/0004-637X/732/2/87 Bibcode: 2011ApJ...732...87C

Cheng, X.; Ding, M. D.; Zhang, J. +2 more

We investigate the distinct properties of two types of flares: eruptive flares associated with coronal mass ejections (CMEs) and confined flares without CMEs. Our study sample includes nine M- and X-class flares, all from the same active region (AR), six of which are confined and three others which are eruptive. The confined flares tend to be more…

2011 The Astrophysical Journal
SOHO 84
Variations in the Axisymmetric Transport of Magnetic Elements on the Sun: 1996-2010
DOI: 10.1088/0004-637X/729/2/80 Bibcode: 2011ApJ...729...80H

Hathaway, David H.; Rightmire, Lisa

We measure the axisymmetric transport of magnetic flux on the Sun by cross-correlating narrow strips of data from line-of-sight magnetograms obtained at a 96 minute cadence by the MDI instrument on the ESA/NASA SOHO spacecraft and then averaging the flow measurements over each synodic rotation of the Sun. Our measurements indicate that the axisymm…

2011 The Astrophysical Journal
SOHO 84