Search Publications

A Magnified View of the Kinematics and Morphology of RCSGA 032727-132609: Zooming in on a Merger at z = 1.7
DOI: 10.1088/0004-637X/781/2/61 Bibcode: 2014ApJ...781...61W

Rigby, Jane R.; Sharon, Keren; Gladders, Michael D. +1 more

We present a detailed analysis of multi-wavelength Hubble Space Telescope/Wide Field Camera 3 (WFC3) imaging and Keck/OSIRIS near-infrared adaptive optics-assisted integral field spectroscopy for a highly magnified lensed galaxy at z = 1.70. This young starburst is representative of ultraviolet-selected star-forming galaxies (SFGs) at z ~ 2 and co…

2014 The Astrophysical Journal
eHST 67
Interstellar and Ejecta Dust in the Cas A Supernova Remnant
DOI: 10.1088/0004-637X/786/1/55 Bibcode: 2014ApJ...786...55A

Arendt, Richard G.; Hwang, Una; Rho, Jeonghee +2 more

Infrared continuum observations provide a means of investigating the physical composition of the dust in the ejecta and swept up medium of the Cas A supernova remnant (SNR). Using low-resolution Spitzer IRS spectra (5-35 µm), and broad-band Herschel PACS imaging (70, 100, and 160 µm), we identify characteristic dust spectra, associated…

2014 The Astrophysical Journal
Herschel 67
A Molecular Line Scan in the Hubble Deep Field North
DOI: 10.1088/0004-637X/782/2/78 Bibcode: 2014ApJ...782...78D

Daddi, E.; Maiolino, R.; Menten, K. M. +20 more

We present a molecular line scan in the Hubble Deep Field North (HDF-N) that covers the entire 3 mm window (79-115 GHz) using the IRAM Plateau de Bure Interferometer. Our CO redshift coverage spans z <~ 0.45, 1 <~ z <~ 1.9 and all z >~ 2. We reach a CO detection limit that is deep enough to detect essentially all z > 1 CO lines repo…

2014 The Astrophysical Journal
eHST 66
The Black Hole Mass of NGC 4151. II. Stellar Dynamical Measurement from Near-infrared Integral Field Spectroscopy
DOI: 10.1088/0004-637X/791/1/37 Bibcode: 2014ApJ...791...37O

Peterson, Bradley M.; Pogge, Richard W.; Storchi-Bergmann, Thaisa +8 more

We present a revised measurement of the mass of the central black hole (M BH ) in the Seyfert 1 galaxy NGC 4151. The new stellar dynamical mass measurement is derived by applying an axisymmetric orbit-superposition code to near-infrared integral field data obtained using adaptive optics with the Gemini Near-infrared Integral Field Spect…

2014 The Astrophysical Journal
eHST 66
New Evidence for a Substellar Luminosity Problem: Dynamical Mass for the Brown Dwarf Binary Gl 417BC
DOI: 10.1088/0004-637X/790/2/133 Bibcode: 2014ApJ...790..133D

Dupuy, Trent J.; Ireland, Michael J.; Liu, Michael C.

We present new evidence for a problem with cooling rates predicted by substellar evolutionary models that implies that model-derived masses in the literature for brown dwarfs and directly imaged planets may be too high. Based on our dynamical mass for Gl 417BC (L4.5+L6) and a gyrochronology system age from its young, solar-type host star, commonly…

2014 The Astrophysical Journal
eHST 66
Observational Characteristics of Coronal Mass Ejections without Low-coronal Signatures
DOI: 10.1088/0004-637X/795/1/49 Bibcode: 2014ApJ...795...49D

Berghmans, D.; Seaton, D. B.; D'Huys, E. +1 more

Solar eruptions are usually associated with a variety of phenomena occurring in the low corona before, during, and after the onset of eruption. Though easily visible in coronagraph observations, so-called stealth coronal mass ejections (CMEs) do not obviously exhibit any of these low-coronal signatures. The presence or absence of distinct low-coro…

2014 The Astrophysical Journal
PROBA-2 SOHO 66
New Evidence for Efficient Collisionless Heating of Electrons at the Reverse Shock of a Young Supernova Remnant
DOI: 10.1088/0004-637X/780/2/136 Bibcode: 2014ApJ...780..136Y

Petre, Robert; Yamaguchi, Hiroya; Hughes, John P. +7 more

Although collisionless shocks are ubiquitous in astrophysics, certain key aspects of them are not well understood. In particular, the process known as collisionless electron heating, whereby electrons are rapidly energized at the shock front, is one of the main open issues in shock physics. Here, we present the first clear evidence for efficient c…

2014 The Astrophysical Journal
Suzaku 65
The Evolution of Galaxy Size and Morphology at z ~ 0.5-3.0 in the GOODS-N Region with Hubble Space Telescope/WFC3 Data
DOI: 10.1088/0004-637X/785/1/18 Bibcode: 2014ApJ...785...18M

Kajisawa, Masaru; Morishita, Takahiro; Ichikawa, Takashi

We analyze the recently released Hubble Space Telescope/Wide Field Camera 3 IR images in the GOODS-N region to study the formation and evolution of quiescent galaxies (QGs). After examining the reliability of two-dimensional light profiles with artificial galaxies, we obtain the morphological parameters with Sérsic profile of 299 QGs and 1083 star…

2014 The Astrophysical Journal
eHST 65
WISE Y Dwarfs as Probes of the Brown Dwarf-Exoplanet Connection
DOI: 10.1088/0004-637X/783/2/68 Bibcode: 2014ApJ...783...68B

Cushing, Michael C.; Kirkpatrick, J. Davy; Gelino, Christopher R. +5 more

We have determined astrometric positions for 15 WISE-discovered late-type brown dwarfs (six T8-9 and nine Y dwarfs) using the Keck-II telescope, the Spitzer Space Telescope, and the Hubble Space Telescope. Combining data from 8 to 20 epochs we derive parallactic and proper motions for these objects, which puts the majority within 15 pc. For ages g…

2014 The Astrophysical Journal
eHST 65
Winds of Low-metallicity OB-type Stars: HST-COS Spectroscopy in IC 1613
DOI: 10.1088/0004-637X/788/1/64 Bibcode: 2014ApJ...788...64G

Garcia, Miriam; Herrero, Artemio; Najarro, Francisco +2 more

We present the first quantitative ultraviolet spectroscopic analysis of resolved OB stars in IC 1613. Because of its alleged very low metallicity (lsim1/10 Z , from H II regions), studies in this Local Group dwarf galaxy could become a significant step forward from the Small Magellanic Cloud (SMC) toward the extremely metal-poor massiv…

2014 The Astrophysical Journal
IUE eHST 65