Search Publications

Short versus Long and Collapsars versus Non-collapsars: A Quantitative Classification of Gamma-Ray Bursts
DOI: 10.1088/0004-637X/764/2/179 Bibcode: 2013ApJ...764..179B

Piran, Tsvi; Bromberg, Omer; Nakar, Ehud +1 more

Gamma-ray bursts (GRBs) are traditionally divided into long and short according to their durations (lg2 s). It was generally believed that this reflects a different physical origin: collapsars (long) and non-collapsars (short). We have recently shown that the duration distribution of collapsars is flat, namely, independent of the duration, at shor…

2013 The Astrophysical Journal
INTEGRAL 207
Accretion Rates for T Tauri Stars Using Nearly Simultaneous Ultraviolet and Optical Spectra
DOI: 10.1088/0004-637X/767/2/112 Bibcode: 2013ApJ...767..112I

Edwards, Suzan; Brown, Alexander; Calvet, Nuria +9 more

We analyze the accretion properties of 21 low-mass T Tauri stars using a data set of contemporaneous near-UV (NUV) through optical observations obtained with the Hubble Space Telescope Imaging Spectrograph and the ground-based Small and Medium Aperture Research Telescope System, a unique data set because of the nearly simultaneous broad wavelength…

2013 The Astrophysical Journal
eHST 207
Dust in the Polar Region as a Major Contributor to the Infrared Emission of Active Galactic Nuclei
DOI: 10.1088/0004-637X/771/2/87 Bibcode: 2013ApJ...771...87H

Hönig, S. F.; Kishimoto, M.; Tristram, K. R. W. +7 more

Dust around active galactic nuclei (AGNs) is distributed over a wide range of spatial scales and can be observed in the infrared (IR). It is generally assumed that the distribution on parsec scales forms a geometrically and optically thick entity in the equatorial plane around the accretion disk and broad-line region—dubbed "dust torus"—that emits…

2013 The Astrophysical Journal
AKARI 205
The Bimodal Metallicity Distribution of the Cool Circumgalactic Medium at z <~ 1
DOI: 10.1088/0004-637X/770/2/138 Bibcode: 2013ApJ...770..138L

Lehner, N.; Prochaska, J. X.; Fox, A. J. +7 more

We assess the metal content of the cool (~104 K) circumgalactic medium (CGM) about galaxies at z <~ 1 using an H I-selected sample of 28 Lyman limit systems (LLS; defined here as absorbers with 16.2 <~ log N H I <~ 18.5) observed in absorption against background QSOs by the Cosmic Origins Spectrograph on board the H…

2013 The Astrophysical Journal
eHST 204
Stellar Kinematics of z ~ 2 Galaxies and the Inside-out Growth of Quiescent Galaxies
DOI: 10.1088/0004-637X/771/2/85 Bibcode: 2013ApJ...771...85V

van Dokkum, Pieter G.; Franx, Marijn; Bezanson, Rachel +6 more

Using stellar kinematics measurements, we investigate the growth of massive, quiescent galaxies from z ~ 2 to today. We present X-Shooter spectra from the UV to NIR and dynamical mass measurements of five quiescent massive (>1011 M ) galaxies at z ~ 2. This triples the sample of z > 1.5 galaxies with well-constrained (…

2013 The Astrophysical Journal
eHST 202
The SL2S Galaxy-scale Lens Sample. IV. The Dependence of the Total Mass Density Profile of Early-type Galaxies on Redshift, Stellar Mass, and Size
DOI: 10.1088/0004-637X/777/2/98 Bibcode: 2013ApJ...777...98S

Treu, Tommaso; Gavazzi, Raphaël; Marshall, Philip J. +4 more

We present optical and near-infrared spectroscopy obtained at Keck, Very Large Telescope, and Gemini for a sample of 36 secure strong gravitational lens systems and 17 candidates identified as part of the Strong Lensing Legacy Survey. The deflectors are massive early-type galaxies in the redshift range zd = 0.2-0.8, while the lensed sou…

2013 The Astrophysical Journal
eHST 201
Stellar Diameters and Temperatures. III. Main-sequence A, F, G, and K Stars: Additional High-precision Measurements and Empirical Relations
DOI: 10.1088/0004-637X/771/1/40 Bibcode: 2013ApJ...771...40B

von Braun, Kaspar; White, Russel; Goldfinger, P. J. +13 more

Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main-sequence stars, ranging from spectral types A7 to K0, 5 of which are exoplanet host stars. We derive linear radii, effective temperatures, and absolute luminosities of the stars using Hipparcos parallaxes and measured bolometric fluxes. The new data are combined…

2013 The Astrophysical Journal
Hipparcos 201
Discovery, Progenitor and Early Evolution of a Stripped Envelope Supernova iPTF13bvn
DOI: 10.1088/2041-8205/775/1/L7 Bibcode: 2013ApJ...775L...7C

Kulkarni, S. R.; Cenko, S. Bradley; Wheeler, J. Craig +26 more

The intermediate Palomar Transient Factory reports our discovery of a young supernova, iPTF13bvn, in the nearby galaxy, NGC 5806 (22.5 Mpc). Our spectral sequence in the optical and infrared suggests a Type Ib classification. We identify a blue progenitor candidate in deep pre-explosion imaging within a 2σ error circle of 80 mas (8.7 pc). The cand…

2013 The Astrophysical Journal
eHST 201
The Structure of the Milky Way's Hot Gas Halo
DOI: 10.1088/0004-637X/770/2/118 Bibcode: 2013ApJ...770..118M

Bregman, Joel N.; Miller, Matthew J.

The Milky Way's million degree gaseous halo contains a considerable amount of mass that, depending on its structural properties, can be a significant mass component. In order to analyze the structure of the Galactic halo, we use XMM-Newton Reflection Grating Spectrometer archival data and measure O VII Kα absorption-line strengths toward 26 active…

2013 The Astrophysical Journal
XMM-Newton 200
HST Spectral Mapping of L/T Transition Brown Dwarfs Reveals Cloud Thickness Variations
DOI: 10.1088/0004-637X/768/2/121 Bibcode: 2013ApJ...768..121A

Burrows, Adam; Apai, Dániel; Radigan, Jacqueline +3 more

Most directly imaged giant exoplanets are fainter than brown dwarfs with similar spectra. To explain their relative underluminosity, unusually cloudy atmospheres have been proposed. However, with multiple parameters varying between any two objects, it remained difficult to observationally test this idea. We present a new method, sensitive time-res…

2013 The Astrophysical Journal
eHST 198