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A Multi-wavelength Investigation of RCW175: An H II Region Harboring Spinning Dust Emission
DOI: 10.1088/0004-637X/754/2/94 Bibcode: 2012ApJ...754...94T

Alves, M. I. R.; Davies, R. D.; Davis, R. J. +13 more

Using infrared, radio continuum, and spectral observations, we performed a detailed investigation of the H II region RCW175. We determined that RCW175, which actually consists of two separate H II regions, G29.1-0.7 and G29.0-0.6, is located at a distance of 3.2 ± 0.2 kpc. Based on the observations we infer that the more compact G29.0-0.6 is less …

2012 The Astrophysical Journal
Herschel 42
A Broadband Study of the Emission from the Composite Supernova Remnant MSH 11-62
DOI: 10.1088/0004-637X/749/2/131 Bibcode: 2012ApJ...749..131S

Gelfand, Joseph D.; Temim, Tea; Hughes, John P. +10 more

MSH 11-62 (G291.0-0.1) is a composite supernova remnant for which radio and X-ray observations have identified the remnant shell as well as its central pulsar wind nebula. The observations suggest a relatively young system expanding into a low-density region. Here, we present a study of MSH 11-62 using observations with the Chandra, XMM -Newton, a…

2012 The Astrophysical Journal
XMM-Newton 41
Moderate-luminosity Growing Black Holes from 1.25 < z < 2.7: Varied Accretion in Disk-dominated Hosts
DOI: 10.1088/0004-637X/761/1/75 Bibcode: 2012ApJ...761...75S

Urry, C. M.; Simmons, B. D.; Schawinski, K. +2 more

We compute black hole masses and bolometric luminosities for 57 active galactic nuclei (AGNs) in the redshift range 1.25 <= z <= 2.67, selected from the GOODS-South deep multi-wavelength survey field via their X-ray emission. We determine host galaxy morphological parameters by separating the galaxies from their central point sources in deep…

2012 The Astrophysical Journal
eHST 41
The Evolution of the Rest-frame V-band Luminosity Function from z = 4: A Constant Faint-end Slope over the Last 12 Gyr of Cosmic History
DOI: 10.1088/0004-637X/748/2/126 Bibcode: 2012ApJ...748..126M

Marchesini, Danilo; Stefanon, Mauro; Whitaker, Katherine E. +1 more

We present the rest-frame V-band luminosity function (LF) of galaxies at 0.4 <= z < 4.0, measured from a near-infrared selected sample constructed from the NMBS, the FIRES, the FIREWORKS, and the ultra-deep NICMOS and WFC3 observations in the HDFN, HUDF, and GOODS-CDFS, all having high-quality optical-to-mid-infrared data. This unique sample…

2012 The Astrophysical Journal
eHST 41
Evolution and Hydrodynamics of the Very Broad X-Ray Line Emission in SN 1987A
DOI: 10.1088/0004-637X/752/2/103 Bibcode: 2012ApJ...752..103D

Haberl, F.; Sturm, R.; Dwarkadas, V. V. +2 more

Observations of SN 1987A by the Chandra High Energy Transmission Grating (HETG) in 1999 and the XMM-Newton Reflection Grating Spectrometer (RGS) in 2003 show very broad (v-b) lines with a full width at half-maximum (FWHM) of order 104 km s-1 at these times the blast wave (BW) was primarily interacting with the H II region aro…

2012 The Astrophysical Journal
XMM-Newton 41
The A2667 Giant Arc at z = 1.03: Evidence for Large-Scale Shocks at High Redshift
DOI: 10.1088/0004-637X/759/1/66 Bibcode: 2012ApJ...759...66Y

Swinbank, A. M.; Richard, J.; Yuan, T. -T. +1 more

We present the spatially resolved emission line ratio properties of a ~1010 M star-forming galaxy at redshift z = 1.03. This galaxy is gravitationally lensed as a triple-image giant arc behind the massive lensing cluster A2667. The main image of the galaxy has magnification factors of 14 ± 2.1 in flux and ~2 × 7 in area, yi…

2012 The Astrophysical Journal
eHST 41
CANDELS: Correlations of Spectral Energy Distributions and Morphologies with Star formation Status for Massive Galaxies at z ~ 2
DOI: 10.1088/0004-637X/752/2/134 Bibcode: 2012ApJ...752..134W

Ferguson, Henry C.; Hathi, Nimish P.; Lucas, Ray A. +17 more

We present a study on spectral energy distributions, morphologies, and star formation for an IRAC-selected extremely red object sample in the GOODS Chandra Deep Field-South. This work was enabled by new HST/WFC3 near-IR imaging from the CANDELS survey as well as the deepest available X-ray data from Chandra 4 Ms observations. This sample consists …

2012 The Astrophysical Journal
eHST 41
High-resolution X-Ray Spectroscopy of the Galactic Supernova Remnant Puppis A with XMM-Newton/RGS
DOI: 10.1088/0004-637X/756/1/49 Bibcode: 2012ApJ...756...49K

Katsuda, Satoru; Petre, Robert; Uchida, Hiroyuki +6 more

We present high-resolution X-ray spectra of cloud-shock interaction regions in the eastern and northern rims of the Galactic supernova remnant Puppis A, using the Reflection Grating Spectrometer on board the XMM-Newton satellite. A number of emission lines including Kα triplets of He-like N, O, and Ne are clearly resolved for the first time. Inten…

2012 The Astrophysical Journal
XMM-Newton 41
Buildup and Release of Magnetic Twist during the X3.4 Solar Flare of 2006 December 13
DOI: 10.1088/0004-637X/760/1/17 Bibcode: 2012ApJ...760...17I

Choe, G. S.; Shiota, D.; Inoue, S. +3 more

We analyze the temporal evolution of the three-dimensional magnetic structure of the flaring active region (AR) NOAA 10930 by using the nonlinear force-free fields extrapolated from the photospheric vector magnetic fields observed by the Solar Optical Telescope on board Hinode. This AR consisted mainly of two types of twisted magnetic field lines:…

2012 The Astrophysical Journal
Hinode SOHO 41
A Study of Heating and Cooling of the ISM in NGC 1097 with Herschel-PACS and Spitzer-IRS
DOI: 10.1088/0004-637X/751/2/144 Bibcode: 2012ApJ...751..144B

Helou, G.; Roussel, H.; Murphy, E. J. +38 more

NGC 1097 is a nearby Seyfert 1 galaxy with a bright circumnuclear starburst ring, a strong large-scale bar, and an active nucleus. We present a detailed study of the spatial variation of the far-infrared (FIR) [C II]158 µm and [O I]63 µm lines and mid-infrared H2 emission lines as tracers of gas cooling, and of the polycycli…

2012 The Astrophysical Journal
Herschel 41