Search Publications

Galactic Center Extinction: Evidence of Metallic Needles in the General Interstellar Medium
DOI: 10.1086/423893 Bibcode: 2004ApJ...611L.109D

Dwek, Eli

The extinction curve derived from Infrared Space Observatory mid-infrared observations of the Galactic center (GC) exhibits a surprisingly flat behavior in the ~3-8 µm region, contrary to the deep minimum expected from standard interstellar dust models consisting of bare silicate and graphite dust particles. We show that this extinction is l…

2004 The Astrophysical Journal
ISO 26
A variable ultra-luminous X-ray source in the colliding galaxy NGC 7714
DOI: 10.1051/0004-6361:20040265 Bibcode: 2004A&A...422..915S

Motch, C.; Soria, R.

We studied the colliding galaxy NGC 7714 with two XMM-Newton observations, six months apart. The galaxy contains two bright X-ray sources: we show that they have different physical nature. The off-nuclear source is an accreting compact object, one of the brightest ultraluminous X-ray sources (ULXs) found to date. It showed spectral and luminosity …

2004 Astronomy and Astrophysics
XMM-Newton 26
GRB 021211 as a Faint Analog of GRB 990123: Exploring the Similarities and Differences in the Optical Afterglows
DOI: 10.1086/425048 Bibcode: 2004AJ....128.1955H

Bloom, J. S.; Caldwell, Nelson; Garnavich, Peter M. +7 more

We present BVRCJHKs photometry of the optical afterglow of the gamma-ray burst GRB 021211 taken at the Magellan, MMT, and WIYN observatories between 0.7 and 50 days after the burst. We find an intrinsic spectral slope at optical and near-infrared wavelengths of 0.69+/-0.14 at 0.87 days. The optical decay during the first day …

2004 The Astronomical Journal
eHST 26
The heliospheric hydrogen wall and astrospheres
DOI: 10.1016/j.asr.2003.01.035 Bibcode: 2004AdSpR..34...66W

Linsky, J. L.; Zank, G. P.; Wood, B. E. +2 more

Charge exchange processes in the outer heliosphere produce a population of hot hydrogen gas within the heliosphere, creating a "hydrogen wall" between the heliopause and bow shock. The heliospheric hydrogen wall scatters Lyα photons passing through it, producing a detectable absorption signature in observations of H I Lyα emission from nearby star…

2004 Advances in Space Research
eHST 26
HST observations of nuclear stellar disks
DOI: 10.1051/0004-6361:20040359 Bibcode: 2004A&A...428..877K

Jaffe, W.; Krajnović, D.

We present observations of four nearby early-type galaxies with previously known nuclear stellar disks using two instruments on-board the Hubble Space Telescope. We observed NGC 4128, NGC 4612, and NGC 5308 with the Wide Field Planetary Camera 2, and the same three galaxies, plus NGC 4570, with the Space Telescope Imaging Spectrograph. We have det…

2004 Astronomy and Astrophysics
eHST 26
Photometric estimates of stellar masses in high-redshift galaxies
DOI: 10.1051/0004-6361:20034276 Bibcode: 2004A&A...418..913B

Berta, S.; Fritz, J.; Franceschini, A. +2 more

We present a new tool for the photometric estimate of stellar masses in distant galaxies. The observed source spectral energy distributions are fitted by combining sets of various simple stellar populations, with different normalizations and different amounts of dust extinction, for a given (Salpeter) IMF. This treatment gives us the best flexibil…

2004 Astronomy and Astrophysics
ISO 26
XMM-Newton Observations of the Extremely Low Accretion Rate Polars SDSS J155331.12+551614.5 and SDSS J132411.57+032050.5
DOI: 10.1086/424540 Bibcode: 2004AJ....128.2443S

Anderson, Scott F.; Brinkmann, J.; Szkody, Paula +6 more

XMM-Newton observations of the polar SDSS J155331.12+551614.5 reveal that all the X-ray flux emerges at energies less than 2 keV. The best fit to the spectrum is with a thermal plasma with kT=0.8 keV plus a 20-90 eV black body, yielding a thermal X-ray luminosity of (8.0-9.5)×1028 ergs s-1. The low temperature and X-ray lumin…

2004 The Astronomical Journal
XMM-Newton 26
Twisted accretion curtains in the intermediate polar FO Aquarii
DOI: 10.1111/j.1365-2966.2004.07542.x Bibcode: 2004MNRAS.349..715E

Cropper, Mark; Hellier, Coel; Ramsay, Gavin +1 more

We report on a ~37-ks XMM-Newton observation of the intermediate polar FO Aquarii, presenting X-ray and ultraviolet data from the EPIC and OM cameras. We find that the system has changed from its previously reported state of disc-overflow accretion to one of purely disc-fed accretion. We detect the previously reported `notch' feature in the X-ray …

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
New properties of energy-dispersed ions in the plasma sheet boundary layer observed by Cluster
DOI: 10.1029/2003JA010277 Bibcode: 2004JGRA..109.5215K

Lundin, R.; Sauvaud, J. -A.; Escoubet, C. P. +18 more

Using multipoint measurements from the Cluster ion spectrometry instruments and the research with adaptive particle imaging detectors, we identified new properties of multiple energy-dispersed ion structures in the plasma sheet boundary layer (PSBL). On 14 February 2001 at about 4.5 RE midnight local time, the PSBL was highly structured…

2004 Journal of Geophysical Research (Space Physics)
Cluster 26
Observations of the Pulsating White Dwarf G 185-32
DOI: 10.1051/0004-6361:20031567 Bibcode: 2004A&A...413..623C

Mazeh, T.; Hansen, C. J.; Kepler, S. O. +32 more

We observed the pulsating hydrogen atmosphere white dwarf G 185-32 with the Whole Earth Telescope in 1992. We report on a weighted Fourier transform of the data detecting 18 periodicities in its light curve. Using the Hubble Space Telescope Faint Object Spectrograph time resolved spectroscopy, and the wavelength dependence of the relative amplitud…

2004 Astronomy and Astrophysics
eHST 26