Search Publications

Radial Flows in Supergranules
DOI: 10.1023/A:1013881213279 Bibcode: 2002SoPh..205...25H

Raymond, J.; Hathaway, D. H.; Han, S. +1 more

We determine the radial component of the supergranular flow velocity by examining the center-to-limb variation of the Doppler velocity signal. We acquire individual Doppler images obtained with the MDI instrument on the SOHO spacecraft and process them to remove the p-mode oscillation signal, the axisymmetric flows, the convective blueshift signal…

2002 Solar Physics
SOHO 45
Discovery of complex narrow X-ray absorption features from the low-mass X-ray binary GX 13+1 with XMM-Newton
DOI: 10.1051/0004-6361:20020192 Bibcode: 2002A&A...385..940S

Parmar, A. N.; Sidoli, L.; Oosterbroek, T. +1 more

We report the detection of a complex of narrow X-ray absorption features from the low-mass X-ray binary GX 13+1 during 3 XMM-Newton observations in 2000 March and April. The features are consistent with being due to resonant scattering of the Kalpha and Kbeta lines of He- and H-like iron (Fe XXV and Fe XXVI) and H-like calcium (Ca XX) Kalpha . Onl…

2002 Astronomy and Astrophysics
XMM-Newton 45
The circumstellar dust shell of the post-AGB star HD 161796
DOI: 10.1051/0004-6361:20020403 Bibcode: 2002A&A...389..547H

Waters, L. B. F. M.; Dominik, C.; Barlow, M. J. +3 more

We have modeled the complete optical to millimeter spectrum of the Post-Asymptotic Giant Branch (Post-AGB) star HD 161796 and its circumstellar dust shell. A full 2-200 mu m spectrum taken with the Infrared Space Observatory was used to constrain the dust properties. A good fit is achieved using only 4 dust components: amorphous silicates, the cry…

2002 Astronomy and Astrophysics
ISO 45
Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters
DOI: 10.1086/338056 Bibcode: 2002ApJ...566..123B

Kneib, J. -P.; Smith, G. P.; Smail, Ian +6 more

We present a morphological analysis of 17 X-ray-selected clusters at z~0.25, imaged uniformly with the Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2). Eight of these clusters comprise a subsample selected for their low X-ray luminosities (<~1044 ergs s-1), called the low-LX sample. The remaining ni…

2002 The Astrophysical Journal
eHST 45
Temperature variations from Hubble Space Telescope imagery and spectroscopy of NGC 7009
DOI: 10.1046/j.1365-8711.2002.05567.x Bibcode: 2002MNRAS.334..777R

Martin, P. G.; Harrington, J. P.; Balick, B. +8 more

We present new Hubble Space Telescope (HST)/WFPC2 imagery and STIS long-slit spectroscopy of the planetary nebula NGC 7009. The primary goal was to obtain high spatial resolution of the intrinsic line ratio [OIII] 4364/5008 and thereby evaluate the electron temperature (Te) and the fractional mean-square Te variation (tA…

2002 Monthly Notices of the Royal Astronomical Society
eHST 44
ISOCAM observations of the Ursa Major cirrus:. Evidence for large abundance variations of small dust grains
DOI: 10.1051/0004-6361:20011074 Bibcode: 2002A&A...381..209M

Miville-Deschênes, M. -A.; Boulanger, F.; Falgarone, E. +1 more

We present mid-IR imaging observations of a high Galactic latitude cirrus obtained with the ISO camera ISOCAM at 6'' angular resolution. The observations were done with two filters LW2 (5-8.5 mu m) and LW3 (12-18 mu m) that measure respectively the aromatic carbon bands and the underlying continuum emission from small dust particles. Three 0.05 sq…

2002 Astronomy and Astrophysics
ISO 44
Testing the line-driven disc wind model: time-resolved ultraviolet spectroscopy of IX Vel and V3885Sgr
DOI: 10.1046/j.1365-8711.2002.05277.x Bibcode: 2002MNRAS.332..127H

Knigge, C.; Long, K. S.; Proga, D. +2 more

To confront the predictions of the most recent line-driven disc wind models with observational evidence, we have obtained Hubble Space Telescope (HST ) STIS (1180-1700Å) echelle spectra of the nova-like variables IX Vel and V3885Sgr at three epochs. The targets were observed in time-tag mode for ~2000s on each occasion, allowing us to study the sp…

2002 Monthly Notices of the Royal Astronomical Society
IUE eHST 44
On the Temperature Structure of M87
DOI: 10.1086/343757 Bibcode: 2002ApJ...580..815M

Molendi, Silvano

We revisit the XMM-Newton observation of M87, focusing our attention on the temperature structure. We find that spectra for most regions of M87 can be adequately fitted by single-temperature models. Only in a few regions, which are cospatial with the east and southwest radio arms, do we find evidence of a second temperature. The cooler component (…

2002 The Astrophysical Journal
XMM-Newton 44
The mineral composition and spatial distribution of the dust ejecta of NGC 6302
DOI: 10.1051/0004-6361:20021119 Bibcode: 2002A&A...394..679K

Waters, L. B. F. M.; Molster, F. J.; Kemper, F. +1 more

We have analysed the full ISO spectrum of the planetary nebula NGC 6302 in order to derive the mineralogical composition of the dust in the nebula. We use an optically thin dust model in combination with laboratory measurements of cosmic dust analogues. We find two main temperature components at about 100 and 50 K respectively, …

2002 Astronomy and Astrophysics
ISO 44
Statistics of galaxy warps in the HDF North and South
DOI: 10.1051/0004-6361:20011672 Bibcode: 2002A&A...382..513R

Battaner, E.; Combes, F.; Jiménez-Vicente, J. +1 more

We present a statistical study of the presence of galaxy warps in the Hubble deep fields. Among a complete sample of 45 edge-on galaxies above a diameter of 1\farcs3, we find 5 galaxies to be certainly warped and 6 galaxies as good candidates. In addition, 4 galaxies reveal a characteristic U-warp. Compared to statistical studies of local warps, a…

2002 Astronomy and Astrophysics
eHST 44