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Two Extrasolar Asteroids with Low Volatile-element Mass Fractions
DOI: 10.1088/0004-637X/750/1/69 Bibcode: 2012ApJ...750...69J

Koester, D.; Zuckerman, B.; Xu, S. +2 more

Using ultraviolet spectra obtained with the Cosmic Origins Spectrograph on the Hubble Space Telescope, we extend our previous ground-based optical determinations of the composition of the extrasolar asteroids accreted onto two white dwarfs, GD 40 and G241-6. Combining optical and ultraviolet spectra of these stars with He-dominated atmospheres, 13…

2012 The Astrophysical Journal
eHST 79
Dynamics of the Solar Magnetic Bright Points Derived from Their Horizontal Motions
DOI: 10.1088/0004-637X/752/1/48 Bibcode: 2012ApJ...752...48C

Chitta, L. P.; Kariyappa, R.; van Ballegooijen, A. A. +2 more

The subarcsecond bright points (BPs) associated with the small-scale magnetic fields in the lower solar atmosphere are advected by the evolution of the photospheric granules. We measure various quantities related to the horizontal motions of the BPs observed in two wavelengths, including the velocity autocorrelation function. A 1 hr time sequence …

2012 The Astrophysical Journal
Hinode 78
LoCuSS: A Dynamical Analysis of X-Ray Active Galactic Nuclei in Local Clusters
DOI: 10.1088/0004-637X/754/2/97 Bibcode: 2012ApJ...754...97H

Finoguenov, A.; Smith, G. P.; Okabe, N. +7 more

We present a study of the distribution of X-ray active galactic nuclei (AGNs) in a representative sample of 26 massive clusters at 0.15 < z < 0.30, combining Chandra observations sensitive to X-ray point sources of luminosity LX ~ 1042 erg s-1 at the cluster redshift with extensive and highly complete spectro…

2012 The Astrophysical Journal
eHST 78
Three-dimensional Evolution of Solar Wind during Solar Cycles 22-24
DOI: 10.1088/0004-637X/751/2/128 Bibcode: 2012ApJ...751..128M

Manoharan, P. K.

This paper presents an analysis of three-dimensional evolution of solar wind density turbulence and speed at various levels of solar activity between solar cycles 22 and 24. The solar wind data used in this study have been obtained from the interplanetary scintillation (IPS) measurements made at the Ooty Radio Telescope, operating at 327 MHz. Resu…

2012 The Astrophysical Journal
SOHO Ulysses 77
Spitzer Observations of Young Red Quasars
DOI: 10.1088/0004-637X/757/2/125 Bibcode: 2012ApJ...757..125U

Lacy, Mark; Schulz, Bernhard; Urrutia, Tanya +3 more

We present mid-infrared spectra and photometry of 13 redshift 0.4 < z < 1 dust reddened quasars obtained with Spitzer IRS and MIPS. We compare properties derived from their infrared spectral energy distributions (intrinsic active galactic nucleus (AGN) luminosity and far-infrared luminosity from star formation) to the host luminosities and m…

2012 The Astrophysical Journal
eHST 77
Kinematic Signatures of Bulges Correlate with Bulge Morphologies and Sérsic Index
DOI: 10.1088/0004-637X/754/1/67 Bibcode: 2012ApJ...754...67F

Bender, Ralf; Drory, Niv; Fisher, David B. +3 more

We use the Marcario Low Resolution Spectrograph at the Hobby-Eberly Telescope to study the kinematics of pseudobulges and classical bulges in the nearby universe. We present major axis rotational velocities, velocity dispersions, and h 3 and h 4 moments derived from high-resolution (σinst ≈ 39 km s-1) sp…

2012 The Astrophysical Journal
eHST 77
IDCS J1433.2+3306: An Infrared-selected Galaxy Cluster at z = 1.89
DOI: 10.1088/0004-637X/756/2/115 Bibcode: 2012ApJ...756..115Z

Dey, Arjun; Gonzalez, Anthony H.; Stanford, S. A. +6 more

We report the discovery of an IR-selected galaxy cluster in the IRAC Distant Cluster Survey (IDCS). New data from the Hubble Space Telescope spectroscopically confirm IDCS J1433.2+3306 at z = 1.89 with robust spectroscopic redshifts for seven members, two of which are based on the 4000 Å break. Detected emission lines such as [O II] and Hβ indicat…

2012 The Astrophysical Journal
eHST 77
Evidence of Wave Damping at Low Heights in a Polar Coronal Hole
DOI: 10.1088/0004-637X/753/1/36 Bibcode: 2012ApJ...753...36H

Hahn, M.; Savin, D. W.; Landi, E.

We have measured the widths of spectral lines from a polar coronal hole using the Extreme Ultraviolet Imaging Spectrometer on board Hinode. Polar coronal holes are regions of open magnetic field and the source of the fast solar wind. We find that the line widths decrease at relatively low heights. Previous observations have attributed such decreas…

2012 The Astrophysical Journal
Hinode 77
A Young Massive Stellar Population around the Intermediate-mass Black Hole ESO 243-49 HLX-1
DOI: 10.1088/2041-8205/747/1/L13 Bibcode: 2012ApJ...747L..13F

Maccarone, T. J.; Knigge, C.; Farrell, S. A. +9 more

We present Hubble Space Telescope and simultaneous Swift X-ray Telescope observations of the strongest candidate intermediate-mass black hole (IMBH) ESO 243-49 HLX-1. Fitting the spectral energy distribution from X-ray to near-infrared wavelengths showed that the broadband spectrum is not consistent with simple and irradiated disk models, but is w…

2012 The Astrophysical Journal
eHST 76
3D-HST Grism Spectroscopy of a Gravitationally Lensed, Low-metallicity Starburst Galaxy at z = 1.847
DOI: 10.1088/2041-8205/758/1/L17 Bibcode: 2012ApJ...758L..17B

Schmidt, Kasper B.; van Dokkum, Pieter G.; Franx, Marijn +17 more

We present Hubble Space Telescope (HST) imaging and spectroscopy of the gravitational lens SL2SJ02176-0513, a cusp arc at z = 1.847. The UV continuum of the lensed galaxy is very blue, which is seemingly at odds with its redder optical colors. The 3D-HST WFC3/G141 near-infrared spectrum of the lens reveals the source of this discrepancy to be extr…

2012 The Astrophysical Journal
eHST 76