Search Publications

Physical Conditions and Star Formation Activity in the Intragroup Medium of Stephan's Quintet
DOI: 10.1086/377445 Bibcode: 2003ApJ...595..665X

Lu, N.; Xu, C. K.; Tuffs, R. J. +2 more

New multiband observations of the famous compact group of galaxies Stephan's Quintet (SQ) are presented and analyzed. These include far-infrared (FIR) images at 60 and 100 µm (ISOPHOT C100 camera), radio continuum images at 1.4 GHz (VLA B configuration) and 4.86 GHz (VLA C configuration), and long-slit optical spectrographs (Palomar 200" tel…

2003 The Astrophysical Journal
ISO 68
A Compact X-Ray Source and Possible X-Ray Jets within the Planetary Nebula Menzel 3
DOI: 10.1086/376979 Bibcode: 2003ApJ...591L..37K

Soker, Noam; Frank, Adam; Balick, Bruce +4 more

We report the discovery, by the Chandra X-Ray Observatory, of X-ray emission from the bipolar planetary nebula Menzel 3. In Chandra CCD imaging, Mz 3 displays hot [~(3-6)×106 K] gas within its twin, coaxial bubbles of optical nebulosity as well as a compact X-ray source at the position of its central star(s). The brightest diffuse X-ray…

2003 The Astrophysical Journal
eHST 68
Modeling the Ne IX Triplet Spectral Region of Capella with the Chandra and XMM-Newton Gratings
DOI: 10.1086/379059 Bibcode: 2003ApJ...598.1277N

Drake, Jeremy J.; Ness, Jan-Uwe; Huenemoerder, David P. +1 more

High-resolution X-ray spectroscopy with the diffraction gratings of Chandra and XMM-Newton offers new chances to study a large variety of stellar coronal phenomena. A popular X-ray calibration target is Capella, which has been observed with all gratings with significant exposure times. We gathered together all available data of the High Energy Tra…

2003 The Astrophysical Journal
XMM-Newton 67
Keck Spectroscopy and Hubble Space Telescope Imaging of GRB 000926: Probing a Host Galaxy at z = 2.038
DOI: 10.1086/367603 Bibcode: 2003ApJ...586..128C

Harrison, F. A.; Galama, T. J.; Bloom, J. S. +4 more

We present early-time Keck spectroscopic observations and late-time Hubble Space Telescope (HST) imaging of GRB 000926. The HST images show a small offset between the optical transient and a bright, compact knot in the host galaxy. Combined with the large equivalent widths measured for metallic absorption lines by the Keck Echellette Spectrograph …

2003 The Astrophysical Journal
eHST 67
Space Telescope Imaging Spectrograph Slitless Observations of Small Magellanic Cloud Planetary Nebulae: A Study on Morphology, Emission-Line Intensity, and Evolution
DOI: 10.1086/378042 Bibcode: 2003ApJ...596..997S

Mutchler, Max; Villaver, Eva; Blades, J. Chris +3 more

A sample of 27 planetary nebulae (PNs) in the Small Magellanic Cloud (SMC) have been observed with the Hubble Space Telescope Imaging Spectrograph (HST/STIS) to determine their morphology, size, and the spatial variation of the ratios of bright emission lines. The morphologies of SMC PNs are similar to those of LMC and Galactic PNs. However, only …

2003 The Astrophysical Journal
eHST 66
Discovery of Two Distant Type Ia Supernovae in the Hubble Deep Field-North with the Advanced Camera for Surveys
DOI: 10.1086/374797 Bibcode: 2003ApJ...589..693B

White, Richard L.; Broadhurst, Tom; Franx, Marijn +30 more

We present observations of the first two supernovae discovered with the recently installed Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST). The supernovae were found in Wide Field Camera images of the Hubble Deep Field-North taken with the F775W, F850LP, and G800L optical elements as part of the ACS guaranteed time observatio…

2003 The Astrophysical Journal
eHST 66
The Phase Coherence of Light from Extragalactic Sources: Direct Evidence against First-Order Planck-Scale Fluctuations in Time and Space
DOI: 10.1086/374350 Bibcode: 2003ApJ...585L..77L

Lieu, Richard; Hillman, Lloyd W.

We present a method of directly testing whether time continues to have its usual meaning on scales of <=tP=(ℏG/c5)1/2~5.4×10-44 s, the Planck time. According to quantum gravity, the time t of an event cannot be determined more accurately than a standard deviation of the form σt/t=a0

2003 The Astrophysical Journal
eHST 66
Further Evidence for Chemical Fractionation from Ultraviolet Observations of Carbon Monoxide
DOI: 10.1086/375483 Bibcode: 2003ApJ...591..986F

Andersson, B. -G.; van Dishoeck, Ewine F.; Federman, S. R. +4 more

Ultraviolet absorption from interstellar 12CO and 13CO was detected toward ρ Oph A and χ Oph. The measurements were obtained at medium resolution with the Goddard High Resolution Spectrograph on the Hubble Space Telescope. Column density ratios, N(12CO)/N(13CO), of 125+/-23 and 117+/-35 were derived for …

2003 The Astrophysical Journal
eHST 65
Follow-Up Hubble Space Telescope/Space Telescope Imaging Spectroscopy of Three Candidate Tidal Disruption Events
DOI: 10.1086/375553 Bibcode: 2003ApJ...592...42G

Komossa, S.; Grupe, D.; Halpern, J. P. +2 more

Large-amplitude, high-luminosity, soft X-ray flares were detected by the ROSAT All-Sky Survey in several galaxies with no evidence for Seyfert activity in their ground-based optical spectra. These flares had the properties predicted for a tidal disruption event by a central supermassive black hole: soft X-ray spectrum, timescale of months, and lar…

2003 The Astrophysical Journal
eHST 64
The Nearby Neutron Star RX J0720.4-3125 from Radio to X-Rays
DOI: 10.1086/375052 Bibcode: 2003ApJ...590.1008K

Frail, D. A.; Kulkarni, S. R.; van Kerkwijk, M. H. +3 more

We present radio, optical, ultraviolet, and X-ray observations of the isolated, thermally emitting neutron star RX J0720.4-3125 using the Parkes radio telescope, the Very Large Array, the Hubble Space Telescope, and the Chandra X-Ray Observatory. From these data we show that the optical/UV spectrum of RX J0720.4-3125 is not well fitted by a Raylei…

2003 The Astrophysical Journal
eHST 64