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The Radiated Energy Budget of Chromospheric Plasma in a Major Solar Flare Deduced from Multi-wavelength Observations
DOI: 10.1088/0004-637X/793/2/70 Bibcode: 2014ApJ...793...70M

Chamberlin, Phillip C.; Milligan, Ryan O.; Kerr, Graham S. +7 more

This paper presents measurements of the energy radiated by the lower solar atmosphere, at optical, UV, and EUV wavelengths, during an X-class solar flare (SOL2011-02-15T01:56) in response to an injection of energy assumed to be in the form of nonthermal electrons. Hard X-ray observations from RHESSI were used to track the evolution of the paramete…

2014 The Astrophysical Journal
Hinode 94
Uncovering the Putative B-star Binary Companion of the SN 1993J Progenitor
DOI: 10.1088/0004-637X/790/1/17 Bibcode: 2014ApJ...790...17F

Van Dyk, Schuyler D.; Filippenko, Alexei V.; Chandra, Poonam +9 more

The Type IIb supernova (SN) 1993J is one of only a few stripped-envelope SNe with a progenitor star identified in pre-explosion images. SN IIb models typically invoke H envelope stripping by mass transfer in a binary system. For the case of SN 1993J, the models suggest that the companion grew to 22 M and became a source of ultraviolet…

2014 The Astrophysical Journal
eHST 94
Weighing "El Gordo" with a Precision Scale: Hubble Space Telescope Weak-lensing Analysis of the Merging Galaxy Cluster ACT-CL J0102-4915 at z = 0.87
DOI: 10.1088/0004-637X/785/1/20 Bibcode: 2014ApJ...785...20J

Sifón, Cristóbal; Hughes, John P.; Barrientos, L. Felipe +5 more

We present a Hubble Space Telescope weak-lensing study of the merging galaxy cluster "El Gordo" (ACT-CL J0102-4915) at z = 0.87 discovered by the Atacama Cosmology Telescope (ACT) collaboration as the strongest Sunyaev-Zel'dovich decrement in its ~1000 deg2 survey. Our weak-lensing analysis confirms that ACT-CL J0102-4915 is indeed an e…

2014 The Astrophysical Journal
eHST 93
Rejecting Proposed Dense Matter Equations of State with Quiescent Low-mass X-Ray Binaries
DOI: 10.1088/2041-8205/796/1/L3 Bibcode: 2014ApJ...796L...3G

Guillot, Sebastien; Rutledge, Robert E.

Neutrons stars are unique laboratories for discriminating between the various proposed equations of state of matter at and above nuclear density. One sub-class of neutron stars—those inside quiescent low-mass X-ray binaries (qLMXBs)—produce a thermal surface emission from which the neutron star radius (R NS) can be measured, using the w…

2014 The Astrophysical Journal
XMM-Newton 93
The Solar Internetwork. I. Contribution to the Network Magnetic Flux
DOI: 10.1088/0004-637X/797/1/49 Bibcode: 2014ApJ...797...49G

Gošić, M.; Bellot Rubio, L. R.; Katsukawa, Y. +2 more

The magnetic network (NE) observed on the solar surface harbors a sizable fraction of the total quiet Sun flux. However, its origin and maintenance are not well known. Here we investigate the contribution of internetwork (IN) magnetic fields to the NE flux. IN fields permeate the interior of supergranular cells and show large emergence rates. We u…

2014 The Astrophysical Journal
Hinode 93
Reverberation Mapping of the Seyfert 1 Galaxy NGC 7469
DOI: 10.1088/0004-637X/795/2/149 Bibcode: 2014ApJ...795..149P

Motohara, K.; Skowron, D. M.; Skowron, J. +43 more

A large reverberation-mapping study of the Seyfert 1 galaxy NGC 7469 has yielded emission-line lags for Hβ λ4861 and He II λ4686 and a central black hole mass measurement M BH ≈ 1 × 107 M , consistent with previous measurements. A very low level of variability during the monitoring campaign precluded meeting our o…

2014 The Astrophysical Journal
IUE 92
A Blue Point Source at the Location of Supernova 2011dh
DOI: 10.1088/2041-8205/793/2/L22 Bibcode: 2014ApJ...793L..22F

Van Dyk, Schuyler D.; Nomoto, Ken'ichi; Quimby, Robert M. +7 more

We present Hubble Space Telescope (HST) observations of the field of the Type IIb supernova (SN) 2011dh in M51 performed at ≈1161 rest-frame days after explosion using the Wide Field Camera 3 and near-UV filters F225W and F336W. A star-like object is detected in both bands and the photometry indicates it has negative (F225W - F336W) color. The obs…

2014 The Astrophysical Journal
eHST 91
Resolved Imaging of the HR 8799 Debris Disk with Herschel
DOI: 10.1088/0004-637X/780/1/97 Bibcode: 2014ApJ...780...97M

Macintosh, Bruce; Matthews, Brenda; Marois, Christian +5 more

We present Herschel far-infrared and submillimeter maps of the debris disk associated with the HR 8799 planetary system. We resolve the outer disk emission at 70, 100, 160, and 250 µm and detect the disk at 350 and 500 µm. A smooth model explains the observed disk emission well. We observe no obvious clumps or asymmetries associated wi…

2014 The Astrophysical Journal
Herschel 90
Ceci N'est Pas a Globular Cluster: The Metallicity Distribution of the Stellar System Terzan 5
DOI: 10.1088/0004-637X/795/1/22 Bibcode: 2014ApJ...795...22M

Dalessandro, E.; Massari, D.; Valenti, E. +9 more

We present new determinations of the iron abundance for 220 stars belonging to the stellar system Terzan 5 in the Galactic bulge. The spectra have been acquired with FLAMES at the Very Large Telescope of the European Southern Observatory and DEIMOS at the Keck II Telescope. This is by far the largest spectroscopic sample of stars ever observed in …

2014 The Astrophysical Journal
eHST 90
Linking Lyα and Low-ionization Transitions at Low Optical Depth
DOI: 10.1088/2041-8205/791/2/L19 Bibcode: 2014ApJ...791L..19J

Oey, M. S.; Jaskot, A. E.

We suggest that low optical depth in the Lyman continuum (LyC) may relate the Lyα emission, C II and Si II absorption, and C II* and Si II* emission seen in high-redshift galaxies. We base this analysis on Hubble Space Telescope Cosmic Origins Spectrograph spectra of four Green Pea (GP) galaxies, which may be analogs of z > 2 Lyα emitters (LAEs…

2014 The Astrophysical Journal
eHST 89