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On the X-Ray Variability of Magnetar 1RXS J170849.0-400910
DOI: 10.1088/0004-637X/783/2/99 Bibcode: 2014ApJ...783...99S

Gehrels, N.; Kennea, J. A.; Beardmore, A. P. +4 more

We present a long-term X-ray flux and spectral analysis for 1RXS J170849.0-400910 using the Swift/X-Ray Telescope spanning over eight years from 2005 to 2013. We also analyze two observations from Chandra and XMM in the period from 2003 to 2004. In this ten-year period, 1RXS J170849.0-400910 displayed several rotational glitches. Previous studies …

2014 The Astrophysical Journal
XMM-Newton 12
Abundance Patterns in the Interstellar Medium of Early-type Galaxies Observed with Suzaku
DOI: 10.1088/0004-637X/783/1/8 Bibcode: 2014ApJ...783....8K

Matsushita, Kyoko; Tamagawa, Toru; Nagino, Ryo +1 more

We have analyzed 17 early-type galaxies, 13 ellipticals and 4 S0 galaxies, observed with Suzaku, and investigated metal abundances (O, Mg, Si, and Fe) and abundance ratios (O/Fe, Mg/Fe, and Si/Fe) in the interstellar medium (ISM). The emission from each on-source region, which is four times the effective radius, r e, is reproduced with …

2014 The Astrophysical Journal
Suzaku 12
Photon-dominated Region Modeling of the [C I], [C II], and CO Line Emission from a Boundary in the Taurus Molecular Cloud
DOI: 10.1088/0004-637X/795/1/26 Bibcode: 2014ApJ...795...26O

Goldsmith, Paul F.; Pineda, Jorge L.; Orr, Matthew E.

We present [C I] and [C II] observations of a linear edge region in the Taurus molecular cloud, and model this region as a cylindrically symmetric photon-dominated region (PDR) exposed to a low-intensity UV radiation field. The sharp, long profile of the linear edge makes it an ideal case to test PDR models and determine cloud parameters. We compa…

2014 The Astrophysical Journal
Herschel 12
The Rest-frame Ultraviolet Structure of 0.5 < z < 1.5 Galaxies
DOI: 10.1088/0004-637X/791/1/18 Bibcode: 2014ApJ...791...18B

Koekemoer, Anton M.; Ravindranath, Swara; Gardner, Jonathan P. +8 more

We present the rest-frame UV wavelength dependence of the Petrosian-like half-light radius (r 50), and the concentration parameter for a sample of 198 star-forming galaxies at 0.5 < z < 1.5. We find a ~5% decrease in r 50 from 1500 Å to 3000 Å, with half-light radii at 3000 Å ranging from 0.6 kpc to 6 kpc. We also find …

2014 The Astrophysical Journal
eHST 12
Panchromatic Hubble Andromeda Treasury. IX. A Photometric Survey of Planetary Nebulae in M31
DOI: 10.1088/0004-637X/792/2/121 Bibcode: 2014ApJ...792..121V

Williams, Benjamin F.; Gordon, Karl D.; Caldwell, Nelson +8 more

We search the Hubble Space Telescope (HST) Advanced Camera for Surveys and Wide Field Camera 3 broadband imaging data from the Panchromatic Hubble Andromeda Treasury (PHAT) survey to identify detections of cataloged planetary nebulae (PNs). Of the 711 PNs currently in the literature within the PHAT footprint, we find 467 detected in the broadband.…

2014 The Astrophysical Journal
eHST 12
Spitzer IRS Observations of the XA Region in the Cygnus Loop Supernova Remnant
DOI: 10.1088/0004-637X/787/1/3 Bibcode: 2014ApJ...787....3S

Blair, William P.; Raymond, John C.; Borkowski, Kazimierz J. +5 more

We report on spectra of two positions in the XA region of the Cygnus Loop supernova remnant obtained with the InfraRed Spectrograph on the Spitzer Space Telescope. The spectra span the 10-35 µm wavelength range, which contains a number of collisionally excited forbidden lines. These data are supplemented by optical spectra obtained at the Wh…

2014 The Astrophysical Journal
IUE 12
Improved Determination of the Atmospheric Parameters of the Pulsating sdB Star Feige 48
DOI: 10.1088/0004-637X/788/1/65 Bibcode: 2014ApJ...788...65L

Latour, M.; Chayer, P.; Green, E. M. +2 more

As part of a multifaceted effort to better exploit the asteroseismological potential of the pulsating sdB star Feige 48, we present an improved spectroscopic analysis of that star based on new grids of NLTE, fully line-blanketed model atmospheres. To that end, we gathered four high signal-to-noise ratio time-averaged optical spectra of varying spe…

2014 The Astrophysical Journal
eHST 12
Nature versus Nurture: Luminous Blue Variable Nebulae in and near Massive Stellar Clusters at the Galactic Center
DOI: 10.1088/0004-637X/785/2/120 Bibcode: 2014ApJ...785..120L

Morris, M. R.; Lau, R. M.; Herter, T. L. +1 more

Three luminous blue variables (LBVs) are located in and near the Quintuplet Cluster at the Galactic center: the Pistol Star, G0.120-0.048, and qF362. We present imaging at 19, 25, 31, and 37 µm of the region containing these three LBVs, obtained with SOFIA using FORCAST. We argue that Pistol and G0.120-0.048 are identical "twins" that exhibi…

2014 The Astrophysical Journal
ISO 12
An Optical-Near-IR Study of a Triplet of Super Star Clusters in the Starburst Core of M82
DOI: 10.1088/0004-637X/789/2/94 Bibcode: 2014ApJ...789...94W

O'Connell, R. W.; Rosa González, D.; Bastian, N. +8 more

We present HST/STIS optical and Gemini/NIFS near-IR IFU spectroscopy and archival Hubble Space Telescope (HST) imaging of the triplet of super star clusters (A1, A2, and A3) in the core of the M82 starburst. Using model fits to the Space Telescope Imaging Spectrograph (STIS) spectra and the weakness of red supergiant CO absorption features (appear…

2014 The Astrophysical Journal
eHST 11
Properties of M31. IV. Candidate Luminous Blue Variables from PAndromeda
DOI: 10.1088/0004-637X/785/1/11 Bibcode: 2014ApJ...785...11L

Price, P. A.; Bianchi, L.; Chambers, K. C. +16 more

We perform a study on the optical and infrared photometric properties of known luminous blue variables (LBVs) in M31 using a sample of LBV candidates from the Local Group Galaxy Survey by Masset et al. We find that M31 LBV candidates show photometric variability ranging from 0.375 to 1.576 mag in r P1 during a 3 yr time span observed by…

2014 The Astrophysical Journal
eHST 11