Search Publications

Extended Tidal Structure in Two Lyα-emitting Starburst Galaxies
DOI: 10.1086/420868 Bibcode: 2004ApJ...608..768C

Cannon, John M.; Skillman, Evan D.; Östlin, Göran +4 more

We present new Very Large Array (VLA) C-configuration H I imaging of the Lyα-emitting starburst galaxies Tol 1924-416 and IRAS 08339+6517. The effective resolution probes neutral gas structures larger than 4.7 kpc in Tol 1924-416 and larger than 8.1 kpc in IRAS 08339+6517. Both systems are revealed to be tidally interacting: Tol 1924-416 with ESO …

2004 The Astrophysical Journal
eHST 28
The H II Regions of the Damped Lyα Absorber SBS 1543+593
DOI: 10.1086/380094 Bibcode: 2004ApJ...600..613S

Turnshek, David A.; Rao, Sandhya M.; Pettini, Max +3 more

We report new imaging and spectroscopic observations of the damped Lyα absorber (DLA) galaxy SBS 1543+593, a nearby dwarf galaxy whose stellar disk is intersected by the sight line to the bright background QSO HS 1543+5921. Hubble Space Telescope imaging observations with WFPC2 in the F450W and F702W bands are used to measure the DLA galaxy's prop…

2004 The Astrophysical Journal
eHST 28
Quasi-simultaneous XMM-Newton and VLA observation of the non-thermal radio emitter HD 168112 (O5.5III(f+))
DOI: 10.1051/0004-6361:20041030-1 Bibcode: 2004A&A...420.1061D

Blomme, R.; Rauw, G.; De Becker, M. +8 more

We report the results of a multiwavelength study of the non-thermal radio emitter HD 168112 (O5.5III(f+)). The detailed analysis of two quasi-simultaneous XMM-Newton and VLA observations reveals strong variability of this star both in the X-ray and radio ranges. The X-ray observations separated by five months reveal a decrease of the X-…

2004 Astronomy and Astrophysics
XMM-Newton 28
The spectral energy distributions of the revised 200-mJy sample
DOI: 10.1111/j.1365-2966.2004.07961.x Bibcode: 2004MNRAS.352..673A

Bondi, M.; Browne, I. W. A.; Antón, S. +2 more

We address the question of why low-luminosity radio sources with similar flat radio spectra show a range of optical activity. The investigation is based on the spectral energy distributions (SEDs) of objects from the 200-mJy sample. We gathered new data from the VLA at 43 GHz, from SCUBA in the JCMT at 2000, 1350 and 850 µm, and from the ISO…

2004 Monthly Notices of the Royal Astronomical Society
ISO 28
Characteristics of quasi-static potential structures observed in the auroral return current region by Cluster
DOI: 10.5194/npg-11-709-2004 Bibcode: 2004NPGeo..11..709M

André, M.; Buchert, S.; Kistler, L. M. +6 more

Temporal and spatial characteristics of intense quasi-static electric fields and associated electric potential structures in the return current region are discussed using Cluster observations at geocentric distances of about 5 Earth radii. Results are presented from four Cluster encounters with such acceleration structures to illustrate common as …

2004 Nonlinear Processes in Geophysics
Cluster 28
The X-Ray Spectrum of the z=6.30 QSO SDSS J1030+0524
DOI: 10.1086/423669 Bibcode: 2004ApJ...611L..13F

Farrah, D.; McMahon, R.; Priddey, R. +2 more

We present a deep XMM-Newton observation of the z=6.30 QSO SDSS J1030+0524, the second most distant quasar currently known. The data contain sufficient counts for spectral analysis, demonstrating the ability of XMM-Newton to measure X-ray spectral shapes of z~6 QSOs with integration times >~100 ks. The X-ray spectrum is well fitted by a power l…

2004 The Astrophysical Journal
XMM-Newton 28
Dynamics and Radiation of Young Type-Ia Supernova Remnants: Important Physical Processes
DOI: 10.1134/1.1819492 Bibcode: 2004AstL...30..737S

Lundqvist, P.; Sorokina, E. I.; Blinnikov, S. I. +1 more

We analyze the physical processes that should be taken into account when modeling young type-Ia supernova remnants (SNRs) with ages of several hundred years in which forward (into the interstellar medium) and reverse (into the ejection) shocks propagate. We show that the energy losses in a heavy-element-rich ejection can be significant for SNRs ev…

2004 Astronomy Letters
XMM-Newton 28
A Bias in Optical Observations of High-Redshift Luminous Infrared Galaxies
DOI: 10.1086/381687 Bibcode: 2004ApJ...600L..15C

Le Floc'h, E.; Charmandaris, V.; Mirabel, I. F.

We present evidence for the dramatically different morphology between the rest-frame UV and 7 µm mid-IR emission of VV 114 and Arp 299, two nearby (z~0) violently interacting luminous infrared galaxies (LIRGs). Nearly all LIRGs are interacting systems, and it is currently accepted that they dominate the IR emission at z>1. LIRGs located a…

2004 The Astrophysical Journal
eHST 28
Three-Dimensional Photoionization Structure and Distances of Planetary Nebulae. I. NGC 6369
DOI: 10.1086/421038 Bibcode: 2004ApJ...609..194M

Monteiro, Hektor; Heathcote, Steve; Schwarz, Hugo E. +1 more

We present the results of mapping the planetary nebula NGC 6369 by using multiple long-slit spectra taken with the Cerro Tololo Inter-American Observatory 1.5 m telescope. We create two-dimensional emission-line images from our spectra and use these to derive fluxes for 17 lines, the Hα/Hβ extinction map, the [S II ] line ratio density map, and th…

2004 The Astrophysical Journal
eHST 28
An XMM-Newton view of M101 - I. The luminous X-ray source population
DOI: 10.1111/j.1365-2966.2004.07546.x Bibcode: 2004MNRAS.349..404J

Warwick, R. S.; Roberts, T. P.; Ward, M. J. +2 more

We present the first results of an XMM-Newton EPIC observation of the luminous X-ray source population in the face-on supergiant spiral galaxy M101. We have studied the spectral and temporal properties of the 14 most luminous sources, all of which have intrinsic X-ray luminosities exceeding the Eddington limit for a 1.4-Msolar neutron s…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 28