Search Publications

Identification of iron sulphide grains in protoplanetary disks
DOI: 10.1038/417148a Bibcode: 2002Natur.417..148K

Waters, L. B. F. M.; Mutschke, H.; Henning, T. +8 more

Sulphur is depleted in cold dense molecular clouds with embedded young stellar objects, indicating that most of it probably resides in solid grains. Iron sulphide grains are the main sulphur species in cometary dust particles, but there has been no direct evidence for FeS in astronomical sources, which poses a considerable problem, because sulphur…

2002 Nature
ISO 104
On the intensity contrast of solar photospheric faculae and network elements
DOI: 10.1051/0004-6361:20020500 Bibcode: 2002A&A...388.1036O

Solanki, S. K.; Sanahuja, B.; Ortiz, A. +2 more

Sunspots, faculae and the magnetic network contribute to solar irradiance variations. The contribution due to faculae and the network is of basic importance, but suffers from considerable uncertainty. We determine the contrasts of active region faculae and the network, both as a function of heliocentric angle and magnetogram signal. To achieve thi…

2002 Astronomy and Astrophysics
SOHO 104
Correlated Dynamics of Hot and Cool Plasmas in the Main Phase of a Solar Flare
DOI: 10.1086/340136 Bibcode: 2002ApJ...568L..61K

Wilhelm, K.; Curdt, W.; Dammasch, I. E. +1 more

We report far-ultraviolet observations of a solar limb flare obtained by the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer. At a fixed pointing of the slit above the limb, spectra were simultaneously obtained in several emission lines that covered a wide temperature range from ~104 to ~107 K. The te…

2002 The Astrophysical Journal
SOHO 104
3D Coronal magnetic field from vector magnetograms: non-constant-alpha force-free configuration of the active region NOAA 8151
DOI: 10.1051/0004-6361:20020993 Bibcode: 2002A&A...392.1119R

Amari, T.; Régnier, S.; Kersalé, E.

The Active Region 8151 (AR 8151) observed in February 1998 is the site of an eruptive event associated with a filament and a S-shaped structure, and producing a slow Coronal Mass Ejection (CME). In order to determine how the CME occurs, we compute the 3D coronal magnetic field and we derive some relevant parameters such as the free magnetic energy…

2002 Astronomy and Astrophysics
SOHO 103
The Structure of the Local Interstellar Medium. I. High-Resolution Observations of Fe II, Mg II, and Ca II toward Stars within 100 Parsecs
DOI: 10.1086/338650 Bibcode: 2002ApJS..139..439R

Redfield, Seth; Linsky, Jeffrey L.

High-resolution absorption measurements (λ/Δλ>~100,000) of the resonance lines of Fe II, Mg II, and Ca II are presented for all available observed targets within 100 pc. The Fe II and Mg II spectra were obtained with the Goddard High Resolution Spectrograph (GHRS) and the Space Telescope Imaging Spectrograph (STIS) instruments aboard the Hubble…

2002 The Astrophysical Journal Supplement Series
eHST 103
Ultra-relativistic electrons in Jupiter's radiation belts
DOI: 10.1038/415987a Bibcode: 2002Natur.415..987B

Johnson, W. T. K.; Klein, M.; Hofstadter, M. +18 more

Ground-based observations have shown that Jupiter is a two-component source of microwave radio emission: thermal atmospheric emission and synchrotron emission from energetic electrons spiralling in Jupiter's magnetic field. Later in situ measurements confirmed the existence of Jupiter's high-energy electron-radiation belts, with evidence for elect…

2002 Nature
Cassini 102
Galactic Starburst NGC 3603 from X-Rays to Radio
DOI: 10.1086/340491 Bibcode: 2002ApJ...573..191M

Ptak, A.; Corcoran, M. F.; Brandner, W. +10 more

NGC 3603 is the most massive and luminous visible starburst region in the Galaxy. We present the first Chandra ACIS-I X-ray image and spectra of this dense, exotic object, accompanied by a deep centimeter-wavelength Australia Telescope Compact Array radio image at similar <~1" spatial resolution and Hubble Space Telescope/ground-based optical d…

2002 The Astrophysical Journal
eHST 102
Optical Identification of Multiple Faint X-Ray Sources in the Globular Cluster NGC 6752: Evidence for Numerous Cataclysmic Variables
DOI: 10.1086/339210 Bibcode: 2002ApJ...569..405P

Anderson, Scott F.; Kaspi, Victoria M.; Verbunt, Frank +8 more

We report on the Chandra X-Ray Observatory ACIS-S3 imaging observation of the globular cluster NGC 6752. We detect six X-ray sources within the 10.5" core radius and 13 more within the 115" half-mass radius down to a limiting luminosity of LX~1030 ergs s-1 for cluster sources. We reanalyze archival data from the Hu…

2002 The Astrophysical Journal
eHST 102
New High Proper Motion Stars from the Digitized Sky Survey. I. Northern Stars with 0.5" yr-1<µ<2.0" yr-1 at Low Galactic Latitudes
DOI: 10.1086/341783 Bibcode: 2002AJ....124.1190L

Lépine, Sébastien; Rich, R. Michael; Shara, Michael M.

We have conducted a systematic search for high proper motion stars in the Digitized Sky Survey, in the area of the sky north of -2.8 degrees in declination and within 25 degrees of the Galactic plane. Using the SUPERBLINK software, a powerful automated blink comparator developed by us, we have identified 601 stars in the magnitude range 9<r<…

2002 The Astronomical Journal
Hipparcos 102
Optical Spectroscopy of Metal-rich H II Regions and Circumnuclear Hot Spots in M83 and NGC 3351
DOI: 10.1086/340371 Bibcode: 2002ApJ...572..838B

Bresolin, Fabio; Kennicutt, Robert C., Jr.

We present optical spectroscopy of a sample of metal-rich extragalactic H II regions in the spiral galaxies M83 (NGC 5236), NGC 3351, and NGC 6384. The metal abundance, estimated from semiempirical methods using strong emission lines, is found to be above solar for most of the objects. The sample includes a number of circumnuclear H II regions (ho…

2002 The Astrophysical Journal
eHST 101