Search Publications

An OSIRIS Study of the Gas Kinematics in a Sample of UV-Selected Galaxies: Evidence of "Hot and Bothered" Starbursts in the Local Universe
DOI: 10.1088/0004-637X/699/2/L118 Bibcode: 2009ApJ...699L.118B

Law, David R.; Overzier, Roderik; Schiminovich, David +6 more

We present data from Integral Field Spectroscopy for three supercompact UV-Luminous Galaxies (ScUVLGs). As nearby (z ~ 0.2) compact (R 50 ~ 1-2 kpc) bright Paschen-α sources, with unusually high star formation rates (SFR = 3-100 M sun yr-1), ScUVLGs are an ideal population for studying detailed kinematics and dynam…

2009 The Astrophysical Journal
eHST 35
A Young Super Star Cluster in the Nuclear Region of NGC 253
DOI: 10.1088/0004-637X/697/2/1180 Bibcode: 2009ApJ...697.1180K

McCrady, Nate; Kornei, Katherine A.

We present observations of a massive star cluster near the nuclear region of the nearby starburst galaxy NGC 253. The peak of near-infrared (IR) emission, which is spatially separated by 4'' from the kinematic center of the galaxy, is coincident with a super star cluster whose properties we examine with low-resolution (R ~ 1200) infrared Cerro Tol…

2009 The Astrophysical Journal
eHST 35
Observation of Solar Wind Charge Exchange Emission from Exospheric Material in and Outside Earth's Magnetosheath 2008 September 25
DOI: 10.1088/0004-637X/691/1/372 Bibcode: 2009ApJ...691..372S

Lepri, S. T.; Kuntz, K. D.; Snowden, S. L. +4 more

A long XMM-Newton exposure is used to observe solar wind charge exchange (SWCX) emission from exospheric material in and outside Earth's magnetosheath. The light curve of the O VII (0.5-0.62 keV) band is compared with a model for the expected emission, and while the emission is faint and the light curve has considerable scatter, the correlation is…

2009 The Astrophysical Journal
XMM-Newton 35
Probing The Origins of the C IV and Fe Kα Baldwin Effects
DOI: 10.1088/0004-637X/702/1/767 Bibcode: 2009ApJ...702..767W

Brandt, W. N.; Wu, Jian; Schneider, Donald P. +3 more

We use UV/optical and X-ray observations of 272 radio-quiet Type 1 active galactic nuclei and quasars to investigate the C IV Baldwin Effect (BEff). The UV/optical spectra are drawn from the Hubble Space Telescope, International Ultraviolet Explorer and Sloan Digital Sky Survey archives. The X-ray spectra are from the Chandra and XMM-Newton archiv…

2009 The Astrophysical Journal
IUE eHST 35
A High Yield of New Sightlines for the Study of Intergalactic Helium: Far-UV-Bright Quasars from the SDSS, GALEX, AND HST
DOI: 10.1088/0004-637X/690/2/1181 Bibcode: 2009ApJ...690.1181S

Anderson, Scott F.; Schneider, Donald P.; York, Donald G. +6 more

Investigations of He II Lyα (304 Å rest-frame) absorption toward a half-dozen quasars at z ~ 3-4 have demonstrated the great potential of helium studies of the intergalactic medium, but the current critically small sample size of clean sightlines for the He II Gunn-Peterson test limits confidence in cosmological inferences, and a larger sample is …

2009 The Astrophysical Journal
eHST 35
The Correlation Between X-ray and UV Properties of BAL QSOs
DOI: 10.1088/0004-637X/690/1/1006 Bibcode: 2009ApJ...690.1006F

Zhang, Kai; Wang, Tinggui; Wang, Junxian +4 more

We compile a large sample of broad absorption line (BAL) quasars with X-ray observations from the XMM-Newton archive data and Sloan Digital Sky Survey Data Release 5. The sample consists of 41 BAL QSOs. Among 26 BAL quasars detected in X-ray, spectral analysis is possible for 12 objects. X-ray absorption is detected in all of them. Complementary t…

2009 The Astrophysical Journal
XMM-Newton 35
Non-LTE Modeling of the Near-Ultraviolet Band of Late-Type Stars
DOI: 10.1088/0004-637X/691/2/1634 Bibcode: 2009ApJ...691.1634S

Hauschildt, P. H.; Short, C. Ian

We investigate the ability of both LTE and non-LTE (NLTE) models to fit the near-UV band absolute flux distribution, f λ(λ), and individual spectral line profiles of three standard stars for which high-quality spectrophotometry and high-resolution spectroscopy are available: The Sun (G2 V), Arcturus (K2 III), and Procyon (F5 IV-V). We i…

2009 The Astrophysical Journal
IUE 35
Xmm-Newton Discovery of 2.6 s Pulsations in the Soft Gamma-Ray Repeater SGR 1627-41
DOI: 10.1088/0004-637X/690/2/L105 Bibcode: 2009ApJ...690L.105E

Tiengo, A.; Götz, D.; Mereghetti, S. +6 more

After nearly a decade of quiescence, the soft gamma-ray repeater SGR 1627-41 reactivated on 2008 May 28 with a bursting episode followed by a slowly decaying enhancement of its persistent emission. To search for the still unknown spin period of this SGR taking advantage of its high flux state, we performed on 2008 September 27-28 a 120 ks long X-r…

2009 The Astrophysical Journal
XMM-Newton 35
Hubble Space Telescope Images and KPNO Spectroscopy of the Binary Black Hole Candidate SDSS J153636.22+044127.0
DOI: 10.1088/0004-637X/703/1/930 Bibcode: 2009ApJ...703..930L

Lauer, Tod R.; Boroson, Todd A.

We present Hubble Space Telescope WFPC2/PC images and KPNO 4 m long-slit spectroscopy of the QSO SDSS J153636.22+044127.0, which we advanced as a candidate binary supermassive black hole. The images reveal a close companion coincident with the radio source identified by Wrobel & Laor. It appears to be consistent with a Mg ~ -21.4 el…

2009 The Astrophysical Journal
eHST 34
Effect of Polarimetric Noise on the Estimation of Twist and Magnetic Energy of Force-Free Fields
DOI: 10.1088/0004-637X/700/1/199 Bibcode: 2009ApJ...700..199T

Gosain, Sanjay; Joshi, Jayant; Tiwari, Sanjiv Kumar +1 more

The force-free parameter α, also known as helicity parameter or twist parameter, bears the same sign as the magnetic helicity under some restrictive conditions. The single global value of α for a whole active region gives the degree of twist per unit axial length. We investigate the effect of polarimetric noise on the calculation of global α value…

2009 The Astrophysical Journal
Hinode 34