Search Publications

Early-type Galaxies with Tidal Debris and Their Scaling Relations in the Spitzer Survey of Stellar Structure in Galaxies (S4G)
DOI: 10.1088/0004-637X/753/1/43 Bibcode: 2012ApJ...753...43K

Ho, Luis C.; Erroz-Ferrer, Santiago; Schinnerer, Eva +21 more

Tidal debris around galaxies can yield important clues on their evolution. We have identified tidal debris in 11 early-type galaxies (T <= 0) from a sample of 65 early types drawn from the Spitzer Survey of Stellar Structure in Galaxies (S4G). The tidal debris includes features such as shells, ripples, and tidal tails. A variety of t…

2012 The Astrophysical Journal
eHST 38
Two-plasma Model for Low Charge State Interplanetary Coronal Mass Ejection Observations
DOI: 10.1088/0004-637X/760/2/141 Bibcode: 2012ApJ...760..141G

Zurbuchen, Thomas H.; Gruesbeck, Jacob R.; Lepri, Susan T.

Recent ACE/SWICS observations have revealed that ~5% of all in situ observed interplanetary coronal mass ejections include time periods with very low charge state ions found to be associated with prominence eruptions. It was also shown that these low charge state ions are often observed concurrently with very high charge state ions. But, the physi…

2012 The Astrophysical Journal
SOHO 38
Quenched Cold Accretion of a Large-scale Metal-poor Filament due to Virial Shocking in the Halo of a Massive z = 0.7 Galaxy
DOI: 10.1088/0004-637X/760/1/68 Bibcode: 2012ApJ...760...68C

Kacprzak, Glenn G.; Spitler, Lee R.; Steidel, Charles C. +4 more

Using HST/COS/STIS and HIRES/Keck high-resolution spectra, we have studied a remarkable H I absorbing complex at z = 0.672 toward the quasar Q1317+277. The H I absorption has a velocity spread of Δv = 1600 km s-1, comprises 21 Voigt profile components, and resides at an impact parameter of D = 58 kpc from a bright, high-mass (log M

2012 The Astrophysical Journal
eHST 38
Resolved Measurements of X CO in NGC 6946
DOI: 10.1088/0004-637X/744/1/42 Bibcode: 2012ApJ...744...42D

Momose, Rieko; Scoville, Nick; Kuno, Nario +9 more

We present the largest sample to date of giant molecular clouds (GMCs) in a substantial spiral galaxy other than the Milky Way. We map the distribution of molecular gas with high resolution and image fidelity within the central 5 kpc of the spiral galaxy NGC 6946 in the 12CO (J = 1-0) transition. By combining observations from the Nobey…

2012 The Astrophysical Journal
eHST 38
New Solar Wind Diagnostic Using Both in Situ and Spectroscopic Measurements
DOI: 10.1088/0004-637X/750/2/159 Bibcode: 2012ApJ...750..159L

Lepri, S. T.; Zurbuchen, T. H.; Landi, E. +1 more

We develop a new diagnostic technique that utilizes, at the same time, two completely different types of observations—in situ determinations of solar wind charge states and high-resolution spectroscopy of the inner solar corona—in order to study the temperature, density, and velocity of the solar wind as a function of height in the inner corona be…

2012 The Astrophysical Journal
Hinode SOHO 38
Temporal and Spectral Evolution in X- and γ-Rays of Magnetar 1E 1547.0-5408 since its 2008 October Outburst: The Discovery of a Transient Hard Pulsed Component after its 2009 January Outburst
DOI: 10.1088/0004-637X/748/2/133 Bibcode: 2012ApJ...748..133K

Kuiper, L.; Hermsen, W.; den Hartog, P. R. +1 more

The magnetar 1E 1547.0-5408 exhibited outbursts in 2008 October and 2009 January. In this paper, we present in great detail the evolution of the temporal and spectral characteristics of the persistent total and pulsed emission of 1E 1547.0-5408 between ~1 and 300 keV starting on 2008 October 3 and ending in 2011 January. We analyzed data collected…

2012 The Astrophysical Journal
INTEGRAL 38
X-Ray Observations of the Young Pulsar J1357—6429 and Its Pulsar Wind Nebula
DOI: 10.1088/0004-637X/744/2/81 Bibcode: 2012ApJ...744...81C

Pavlov, George G.; Kargaltsev, Oleg; Chang, Chulhoon +1 more

We observed the young pulsar J1357—6429 with the Chandra and XMM-Newton observatories. The pulsar spectrum fits well a combination of an absorbed power-law model (Γ = 1.7 ± 0.6) and a blackbody model (kT = 140+60 - 40 eV, R ~ 2 km at the distance of 2.5 kpc). Strong pulsations with pulsed fraction of 42% ± 5%, apparently asso…

2012 The Astrophysical Journal
XMM-Newton 37
Initiation and Development of the White-light and Radio Coronal Mass Ejection on 2001 April 15
DOI: 10.1088/0004-637X/750/2/147 Bibcode: 2012ApJ...750..147D

Pick, M.; Démoulin, P.; Vourlidas, A. +1 more

The 2001 April 15 event was one of the largest of the last solar cycle. A former study established that this event was associated with a coronal mass ejection (CME) observed both at white light and radio frequencies. This radio CME is illuminated by synchrotron emission from relativistic electrons. In this paper, we investigate the relation of the…

2012 The Astrophysical Journal
SOHO 37
The Faint End of the Cluster-galaxy Luminosity Function at High Redshift
DOI: 10.1088/0004-637X/761/2/141 Bibcode: 2012ApJ...761..141M

Wright, Edward L.; Eisenhardt, Peter R. M.; Gonzalez, Anthony H. +7 more

We measure the faint-end slope of the galaxy luminosity function (LF) for cluster galaxies at 1 < z < 1.5 using Spitzer IRAC data. We investigate whether this slope, α, differs from that of the field LF at these redshifts, and with the cluster LF at low redshifts. The latter is of particular interest as low-luminosity galaxies are expected t…

2012 The Astrophysical Journal
eHST 37
A Significant Problem with Using the Amati Relation for Cosmological Purposes
DOI: 10.1088/0004-637X/747/1/39 Bibcode: 2012ApJ...747...39C

Collazzi, Andrew C.; Schaefer, Bradley E.; Goldstein, Adam +1 more

We consider the distribution of many samples of gamma-ray bursts when plotted in a diagram with their bolometric fluence (S bolo) versus the observed photon energy of peak spectral flux (E peak, obs). In this diagram, all bursts that obey the Amati relation (a luminosity relation where the total burst energy has a power-law r…

2012 The Astrophysical Journal
Suzaku 37