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A Self-Consistent Nonlinear Force-Free Solution for a Solar Active Region Magnetic Field
DOI: 10.1088/0004-637X/700/2/L88 Bibcode: 2009ApJ...700L..88W

Régnier, S.; Wheatland, M. S.

Nonlinear force-free solutions for the magnetic field in the solar corona constructed using photospheric vector magnetic field boundary data suffer from a basic problem: the observed boundary data are inconsistent with the nonlinear force-free model. Specifically, there are two possible choices of boundary conditions on vertical current provided b…

2009 The Astrophysical Journal
Hinode SOHO 60
Spitzer View of Young Massive Stars in the Large Magellanic Cloud H II Complex N 44
DOI: 10.1088/0004-637X/695/1/511 Bibcode: 2009ApJ...695..511C

Gordon, Karl D.; Chu, You-Hua; Gruendl, Robert A. +2 more

The H II complex N 44 in the Large Magellanic Cloud (LMC) provides an excellent site to perform a detailed study of star formation in a mild starburst, as it hosts three regions of star formation at different evolutionary stages, and it is not as complicated and confusing as the 30 Doradus giant H II region. We have obtained Spitzer Space Telescop…

2009 The Astrophysical Journal
eHST 60
Revealing the Structure of a Pre-Transitional Disk: The Case of the Herbig F Star SAO 206462 (HD 135344B)
DOI: 10.1088/0004-637X/699/2/1822 Bibcode: 2009ApJ...699.1822G

Ménard, F.; Apai, D.; Hamaguchi, K. +23 more

SAO 206462 (HD 135344B) has previously been identified as a Herbig F star with a circumstellar disk with a dip in its infrared excess near 10 µm. In combination with a low accretion rate estimated from Br γ, it may represent a gapped, but otherwise primordial or "pre-transitional" disk. We test this hypothesis with Hubble Space Telescope cor…

2009 The Astrophysical Journal
ISO eHST 59
Current Buildup in Emerging Serpentine Flux Tubes
DOI: 10.1088/0004-637X/701/2/1911 Bibcode: 2009ApJ...701.1911P

Aulanier, G.; Masson, S.; Pariat, E.

The increase of magnetic flux in the solar atmosphere during active-region formation involves the transport of the magnetic field from the solar convection zone through the lowest layers of the solar atmosphere, through which the plasma β changes from >1 to <1 with altitude. The crossing of this magnetic transition zone requires the magnetic…

2009 The Astrophysical Journal
SOHO 59
The NGC 300 Transient: An Alternative Method for Measuring Progenitor Masses
DOI: 10.1088/0004-637X/703/1/300 Bibcode: 2009ApJ...703..300G

Williams, Benjamin F.; Dolphin, Andrew; Dalcanton, Julianne J. +3 more

We present an alternative technique for measuring the precursor masses of transient events in stars undergoing late stage stellar evolution. We use the well-established techniques of stellar population modeling to age-date the stars surrounding the site of the recent transient event in NGC 300 (NGC 300 OT2008-1). The surrounding stars must share a…

2009 The Astrophysical Journal
eHST 59
Correlated X-Ray and Very High Energy Emission in the Gamma-Ray Binary LS I +61 303
DOI: 10.1088/0004-637X/706/1/L27 Bibcode: 2009ApJ...706L..27A

Maraschi, L.; Covino, S.; Antonelli, L. A. +153 more

The discovery of very high energy (VHE) gamma-ray emitting X-ray binaries has triggered an intense effort to better understand the particle acceleration, absorption, and emission mechanisms in compact binary systems, which provide variable conditions along eccentric orbits. Despite this, the nature of some of these systems, and of the accelerated …

2009 The Astrophysical Journal
XMM-Newton 59
Some Like It Hot: Coronal Heating Observations from Hinode X-ray Telescope and RHESSI
DOI: 10.1088/0004-637X/704/1/863 Bibcode: 2009ApJ...704..863S

Lin, L.; Golub, L.; Schmelz, J. T. +7 more

We have used Hinode X-Ray Telescope observations and RHESSI upper limits together to characterize the differential emission measure (DEM) from a quiescent active region. We find a relatively smooth DEM curve with the expected active region peak at log T = 6.4. We also find a high-temperature component with significant emission measure at log T gsi…

2009 The Astrophysical Journal
Hinode 59
New Observation of Failed Filament Eruptions: The Influence of Asymmetric Coronal Background Fields on Solar Eruptions
DOI: 10.1088/0004-637X/696/1/L70 Bibcode: 2009ApJ...696L..70L

Liu, Y.; Shibata, K.; Lin, H. +3 more

Failed filament eruptions not associated with a coronal mass ejection (CME) have been observed and reported as evidence for solar coronal field confinement on erupting flux ropes. In those events, each filament eventually returns to its origin on the solar surface. In this Letter, a new observation of two failed filament eruptions is reported whic…

2009 The Astrophysical Journal
SOHO 59
Global Star Formation Rate Density over 0.7 < z < 1.9
DOI: 10.1088/0004-637X/696/1/785 Bibcode: 2009ApJ...696..785S

Henry, Alaina; Shim, Hyunjin; Teplitz, Harry +4 more

We determine the global star formation rate (SFR) density at 0.7 < z < 1.9 using emission-line-selected galaxies identified in Hubble Space Telescope-Near Infrared Camera and Multi-Object Spectrograph (HST-NICMOS) grism spectroscopy observations. Observing in a pure parallel mode throughout HST Cycles 12 and 13, our survey covers ~104 arcmin…

2009 The Astrophysical Journal
eHST 57
Simultaneous Multiwavelength Observations of Markarian 421 During Outburst
DOI: 10.1088/0004-637X/703/1/169 Bibcode: 2009ApJ...703..169A

Maraschi, L.; Covino, S.; Antonelli, L. A. +226 more

We report on the results of two coordinated multiwavelength campaigns that focused on the blazar Markarian 421 during its 2006 and 2008 outbursts. These campaigns obtained UV and X-ray data using the XMM-Newton satellite, while the gamma-ray data were obtained utilizing three imaging atmospheric Cerenkov telescopes, the Whipple 10 m telescope and …

2009 The Astrophysical Journal
XMM-Newton 57