Search Publications

Hot Gas in the Circumstellar Bubble S308
DOI: 10.1086/379607 Bibcode: 2003ApJ...599.1189C

Guerrero, Martín A.; Chu, You-Hua; Gruendl, Robert A. +2 more

S308 is a circumstellar bubble blown by the WN4 star HD 50896. It is one of the only two single-star bubbles that show detectable diffuse X-ray emission. We have obtained XMM-Newton EPIC observations of the northwest quadrant of S308. The diffuse X-ray emission shows a limb-brightened morphology, with a clear gap extending from the outer edge of t…

2003 The Astrophysical Journal
XMM-Newton 56
Evidence for an Intermediate-Age, Metal-rich Population of Globular Clusters in NGC 4365
DOI: 10.1086/346219 Bibcode: 2003ApJ...585..767L

Forbes, Duncan A.; Brodie, Jean P.; Beasley, Michael A. +4 more

We present spectroscopy for globular clusters (GCs) in the elliptical galaxy NGC 4365, obtained with the Low-Resolution Imaging Spectrograph on the Keck I telescope. Previous studies have shown that the optical color distribution of GCs in NGC 4365 lacks the bimodal structure that is common in globular cluster systems, showing only a single broad …

2003 The Astrophysical Journal
eHST 56
Chandra Observation of the Edge-on Galaxy NGC 3556 (M108): Violent Galactic Disk-Halo Interaction Revealed
DOI: 10.1086/379010 Bibcode: 2003ApJ...598..969W

Wang, Q. Daniel; Irwin, Judith A.; Chaves, Tara

We present a 60 ks Chandra ACIS-S observation of the isolated edge-on spiral galaxy NGC 3556, together with a multiwavelength analysis of various discrete X-ray sources and diffuse X-ray features. Among 33 discrete X-ray sources detected within the IB=25 mag arcsec-2 isophote ellipse of the galaxy, we identify a candidate for…

2003 The Astrophysical Journal
eHST 55
X-Ray Evidence of a Buried Active Galactic Nucleus in UGC 5101
DOI: 10.1086/379503 Bibcode: 2003ApJ...596L.167I

Nakagawa, Takao; Imanishi, Masatoshi; Terashima, Yuichi +1 more

We present X-ray observations of the ultraluminous infrared galaxy, UGC 5101, thought to contain a buried active galactic nucleus (AGN) based on observations in other wave bands. We detected an absorbed hard component at greater than 3 keV, as well as soft emission in the energy range 0.5-2 keV. The soft X-ray component, possibly due to a modestly…

2003 The Astrophysical Journal
XMM-Newton 55
The Canada-UK Deep Submillimeter Survey. VII. Optical and Near-Infrared Identifications for the 14 Hour Field
DOI: 10.1086/381217 Bibcode: 2003ApJ...597..680W

Clements, D. L.; Dunne, L.; Eales, S. +5 more

We present the multiwavelength identifications for 23 sources in the Canada-UK Deep Submillimeter Survey (CUDSS) 14h field. The identifications have been selected on the basis of radio and near-infrared data, and we argue that, to our observational limits, both are effective at selecting the correct counterparts of the SCUBA sources. We…

2003 The Astrophysical Journal
ISO eHST 55
X-Ray Spectroscopy of the Low-Mass X-Ray Binaries 2S 0918-549 and 4U 1543-624: Evidence for Neon-rich Degenerate Donors
DOI: 10.1086/379188 Bibcode: 2003ApJ...599..498J

Chakrabarty, Deepto; Juett, Adrienne M.

We present high-resolution spectroscopy of the neutron star/low-mass X-ray binaries 2S 0918-549 and 4U 1543-624 with the High Energy Transmission Grating Spectrometer on board the Chandra X-Ray Observatory and the Reflection Grating Spectrometer on board XMM-Newton. Previous low-resolution spectra of both sources showed a broad, linelike feature a…

2003 The Astrophysical Journal
XMM-Newton 55
Simultaneous Ultraviolet and X-Ray Spectroscopy of the Seyfert 1 Galaxy NGC 5548. I. Physical Conditions in the Ultraviolet Absorbers
DOI: 10.1086/376792 Bibcode: 2003ApJ...594..116C

Kaastra, J. S.; Turner, T. J.; Kraemer, S. B. +9 more

We present new UV spectra of the nucleus of the Seyfert 1 galaxy NGC 5548, which we obtained with the Space Telescope Imaging Spectrograph at high spectral resolution, in conjunction with simultaneous Chandra X-Ray Observatory spectra. Taking advantage of the low UV continuum and broad emission-line fluxes, we have determined that the deepest UV a…

2003 The Astrophysical Journal
IUE eHST 55
Hubble Space Telescope Observations of High-Velocity Lyα and Hα Emission from Supernova Remnant 1987A: The Structure and Development of the Reverse Shock
DOI: 10.1086/376725 Bibcode: 2003ApJ...593..809M

Filippenko, Alexei V.; Pun, C. S. J.; Garnavich, Peter +18 more

We present two-dimensional line profiles of high-velocity (~+/-12,000 km s-1) Lyα and Hα emission from supernova remnant 1987A obtained with the Space Telescope Imaging Spectrograph between 1997 September and 2001 September (days 3869-5327 after the explosion). This emission comes from hydrogen in the debris that is excited and ionized …

2003 The Astrophysical Journal
eHST 54
The Ionized Gas and Nuclear Environment in NGC 3783. III. Detection of a Decreasing Radial Velocity in an Intrinsic Ultraviolet Absorber
DOI: 10.1086/377342 Bibcode: 2003ApJ...595..120G

Kaiser, Mary Elizabeth; Brandt, W. N.; Kaspi, Shai +14 more

We report an intrinsic absorber with decreasing outflow velocity in the Seyfert 1 galaxy NGC 3783. This is the first detection of a change in radial velocity in an outflow associated with a Seyfert galaxy. These results are based on measurements from 18 observations with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope, o…

2003 The Astrophysical Journal
eHST 54
Measuring σ8 with Cluster Lensing: Biases from Unrelaxed Clusters
DOI: 10.1086/376747 Bibcode: 2003ApJ...590L..79S

Smith, Graham P.; Smail, Ian; Kneib, Jean-Paul +3 more

We use gravitational lens models and X-ray spectral analysis of 10 X-ray-luminous galaxy clusters at z~=0.2 to study the impact of cluster substructure on attempts to normalize the matter power spectrum. We estimate that unrelaxed clusters are 30% hotter than relaxed clusters, causing σ8 to be overestimated by 20% if the cluster selecti…

2003 The Astrophysical Journal
eHST 54