Search Publications

Elemental Depletions in the Magellanic Clouds and the Evolution of Depletions with Metallicity
DOI: 10.1088/0004-637X/811/2/78 Bibcode: 2015ApJ...811...78T

Meixner, Margaret; Seale, Jonathan; Dwek, Eli +4 more

We present a study of the composition of gas and dust in the Large and Small Magellanic Clouds (LMC and SMC) using UV absorption spectroscopy. We measure P ii and Fe ii along 84 spatially distributed sightlines toward the MCs using archival Far Ultraviolet Spectroscopic Explorer observations. For 16 of those sightlines, we also measure Si ii, Cr i…

2015 The Astrophysical Journal
eHST 58
The VLT SINFONI Mg II Program for Line Emitters (SIMPLE). II. Background Quasars Probing Z ~ 1 Galactic Winds
DOI: 10.1088/0004-637X/804/2/83 Bibcode: 2015ApJ...804...83S

Finley, Hayley; Bouché, Nicolas; Contini, Thierry +3 more

The physical properties of galactic winds are of paramount importance for our understanding of galaxy formation. Fortunately, they can be constrained using background quasars passing near star-forming galaxies (SFGs). From the 14 quasar-galaxy pairs in our Very Large Telescope (VLT)/SINFONI Mg ii Program for Line Emitters sample, we reobserved the…

2015 The Astrophysical Journal
eHST 58
Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z = 3.35: a Detailed Look at an Early Progenitor of Local Giant Ellipticals
DOI: 10.1088/0004-637X/801/2/133 Bibcode: 2015ApJ...801..133M

van Dokkum, Pieter G.; Muzzin, Adam; Labbé, Ivo +10 more

We present the first spectroscopic confirmation of an ultramassive galaxy at redshift z\gt 3 using data from Keck-NIRSPEC, VLT-X-shooter, and GTC-Osiris. We detect strong [O iii] and Lyα emission, and weak [O ii], C iv, and He ii, placing C1-23152 at a spectroscopic redshift of {{z}spec}=3.351. The modeling of the emission-line-correcte…

2015 The Astrophysical Journal
eHST 57
Broadband Radio Polarimetry and Faraday Rotation of 563 Extragalactic Radio Sources
DOI: 10.1088/0004-637X/815/1/49 Bibcode: 2015ApJ...815...49A

Gaensler, B. M.; Franzen, T. M. O.; Anderson, C. S. +1 more

We present a broadband spectropolarimetric survey of 563 discrete, mostly unresolved radio sources between 1.3 and 2.0 GHz using data taken with the Australia Telescope Compact Array. We have used rotation-measure synthesis to identify Faraday-complex polarized sources, those objects whose frequency-dependent polarization behavior indicates the pr…

2015 The Astrophysical Journal
Planck 57
HST Rotational Spectral Mapping of Two L-type Brown Dwarfs: Variability in and out of Water Bands indicates High-altitude Haze Layers
DOI: 10.1088/2041-8205/798/1/L13 Bibcode: 2015ApJ...798L..13Y

Metchev, Stanimir; Showman, Adam P.; Apai, Dániel +13 more

We present time-resolved near-infrared spectroscopy of two L5 dwarfs, 2MASS J18212815+1414010 and 2MASS J15074759-1627386, observed with the Wide Field Camera 3 instrument on the Hubble Space Telescope (HST). We study the wavelength dependence of rotation-modulated flux variations between 1.1 µm and 1.7 µm. We find that the water absor…

2015 The Astrophysical Journal
eHST 57
On the Origin of Mid-latitude Fast Wind: Challenging the Two-state Solar Wind Paradigm
DOI: 10.1088/0004-637X/801/2/100 Bibcode: 2015ApJ...801..100S

Landi, Enrico; Zurbuchen, Thomas H.; Lepri, Susan T. +2 more

The bimodal paradigm of solar wind describes a slow solar wind situated near the heliospheric current sheet while a fast wind overexpands from the poles to fill in the remainder of the heliosphere. In this paper, we challenge this paradigm and focus here on mid-latitude wind using three fast-latitude passes completed by the Ulysses spacecraft. Bas…

2015 The Astrophysical Journal
Ulysses 57
NuSTAR and XMM-Newton Observations of the Extreme Ultraluminous X-Ray Source NGC 5907 ULX1: A Vanishing Act
DOI: 10.1088/0004-637X/799/2/122 Bibcode: 2015ApJ...799..122W

Harrison, F. A.; Stern, D.; Bachetti, M. +15 more

We present results obtained from two broadband X-ray observations of the extreme ultraluminous X-ray source (ULX) NGC 5907 ULX1, known to have a peak X-ray luminosity of ~5 × 1040 erg s-1. These XMM-Newton and NuSTAR observations, separated by only ~4 days, revealed an extreme level of short-term flux variability. In the firs…

2015 The Astrophysical Journal
XMM-Newton 56
New Ultraviolet Extinction Curves for Interstellar Dust in M31
DOI: 10.1088/0004-637X/815/1/14 Bibcode: 2015ApJ...815...14C

Gordon, Karl D.; Fitzpatrick, Edward L.; Bohlin, R. C. +4 more

New low-resolution UV spectra of a sample of reddened OB stars in M31 were obtained with the Hubble Space Telescope/STIS to study the wavelength dependence of interstellar extinction and the nature of the underlying dust grain populations. Extinction curves were constructed for four reddened sightlines in M31 paired with closely matching stellar a…

2015 The Astrophysical Journal
eHST 56
Herschel Galactic Plane Survey of [NII] Fine Structure Emission
DOI: 10.1088/0004-637X/814/2/133 Bibcode: 2015ApJ...814..133G

Goldsmith, Paul F.; Pineda, Jorge L.; Yıldız, Umut A. +1 more

We present the first large-scale high angular resolution survey of ionized nitrogen in the Galactic Plane through emission of its two fine structure transitions ([N ii]) at 122 and 205 µm. The observations were largely obtained with the PACS instrument onboard the Herschel Space Observatory. The lines of sight were in the Galactic plane, fol…

2015 The Astrophysical Journal
Herschel 56
The Galactic 26Al Emission Map as Revealed by INTEGRAL SPI
DOI: 10.1088/0004-637X/801/2/142 Bibcode: 2015ApJ...801..142B

Jourdain, Elisabeth; Roques, Jean-Pierre; Bouchet, Laurent

Diffuse emission is often challenging since it is undetectable by most instruments, which are generally dedicated to point-source studies. The 26Al emission is a good illustration: the only available 26Al map to date has been released, more than 15 yr ago, thanks to the COMPTEL instrument. However, at the present time, the SP…

2015 The Astrophysical Journal
INTEGRAL 56