Search Publications

Flow in streamer boundaries, and streamer stability
DOI: 10.1016/S0273-1177(03)00237-0 Bibcode: 2004AdSpR..33..668S

Suess, S. T.; Nerney, S.

Streamers can extend to many solar radii but the closed field regions, or helmets, reach no higher than 2-4 solar radii. The brightness boundary defining streamers is therefore, a boundary between different flow regimes rather than between static plasma and expanding solar wind. It is reasonable to assume that, this boundary divides fast coronal h…

2004 Advances in Space Research
SOHO 12
Cosmic Helium Production
DOI: 10.1071/AS04015 Bibcode: 2004PASA...21..126F

Flynn, Chris

K-dwarfs are very long lived, slowly evolving stars, so that their present day helium Y and metal content (metallicity Z) is essentially the same as when they were born. K-dwarfs thus contain a fossil record of the amount of helium and metals which has been produced in successive stellar generations over the lifetime of the Galaxy. We here estimat…

2004 Publications of the Astronomical Society of Australia
Hipparcos 12
Proper Motion Objects in the Hubble Deep Field
DOI: 10.1086/421343 Bibcode: 2004ApJ...609..766K

Winget, D. E.; von Hippel, Ted; Mendez, R. A. +1 more

Using the deepest and finest resolution images of the universe acquired with the Hubble Space Telescope and a similar image taken 7 yr later for the Great Observatories Origins Deep Survey, we have derived proper motions for the point sources in the Hubble Deep Field-North. Two faint blue objects, HDF 2234 and HDF 3072, are found to display signif…

2004 The Astrophysical Journal
eHST 12
Far-Ultraviolet Spectroscopy of Star-forming Regions in Nearby Galaxies: Stellar Populations and Abundance Indicators
DOI: 10.1086/421367 Bibcode: 2004AJ....128..211K

Keel, William C.; Holberg, Jay B.; Treuthardt, Patrick M.

We present Far Ultraviolet Spectroscopic Explorer spectroscopy and supporting data for star-forming regions in nearby galaxies, to examine their massive-star content and explore the use of abundance and population indicators in this spectral range for high-redshift galaxies. New far-ultraviolet spectra are shown for four bright H II regions in M33…

2004 The Astronomical Journal
eHST 12
Prelaunch performance evaluation of the cometary experiment MUPUS-TP
DOI: 10.1029/2003JE002192 Bibcode: 2004JGRE..109.7S09M

Kührt, E.; Knollenberg, J.; Spohn, T. +13 more

This paper discusses test results obtained in both laboratory and terrestrial environment conditions for the ``Multipurpose Sensors for Surface and Sub-Surface Science'' Thermal Probe (MUPUS-TP), which has been developed for the European Space Agency Rosetta cometary rendezvous mission. The probe is intended to provide in situ long-term observatio…

2004 Journal of Geophysical Research (Planets)
Rosetta 12
A stratospheric balloon experiment to test the Huygens atmospheric structure instrument (HASI)
DOI: 10.1016/j.pss.2004.02.009 Bibcode: 2004P&SS...52..867F

Patel, M. R.; Fulchignoni, M.; Hathi, B. +15 more

We developed a series of balloon experiments parachuting a 1:1 scale mock-up of the Huygens probe from an altitude just over 30 km to simulate at planetary scale the final part of the descent of the probe through Titan's lower atmosphere. The terrestrial atmosphere represents a natural laboratory where most of the physical parameters meet quite we…

2004 Planetary and Space Science
Huygens 12
Modulation in the solar irradiance due to surface magnetism during cycles 21, 22 and 23
DOI: 10.1051/0004-6361:20047102 Bibcode: 2004A&A...425..301J

Jain, K.; Hasan, S. S.

Magnetic field indices derived from synoptic magnetograms of the Mt. Wilson Observatory, i.e. Magnetic Plage Strength Index (MPSI) and Mt. Wilson Sunspot Index (MWSI), are used to study the effects of surface magnetism on total solar irradiance variability during solar cycles 21, 22 and 23. We find that most of the solar cycle variation in the tot…

2004 Astronomy and Astrophysics
SOHO 12
XMM-Newton spectra of hard spectrum Rosat AGN: X-ray absorption and optical reddening
DOI: 10.1051/0004-6361:20035683 Bibcode: 2004A&A...420..163C

Page, M. J.; Carrera, F. J.; Mittaz, J. P. D.

We present the XMM-Newton spectra of three low-redshift intermediate Seyferts (one Sy 1.5, and two Sy 1.8), from our survey of hard spectrum Rosat sources. The three AGN are well fitted by absorbed powerlaws, with intrinsic nuclear photoelectric absorption from column densities between 1.3 and 4.0 × 1021 cm-2. In the brightes…

2004 Astronomy and Astrophysics
XMM-Newton 12
INTEGRAL observation of 3EG J1736-2908
DOI: 10.1051/0004-6361:20040484 Bibcode: 2004A&A...425...89D

Gehrels, N.; Grandi, P.; Chaty, S. +10 more

The possible identification by INTEGRAL of the EGRET source 3EG J1736-2908 with the active galactic nucleus GRS 1734-292 is discussed. The latter was discovered in 1990 and later identified with a Seyfert 1 galaxy. At the time of the compilation of the 3rd EGRET Catalog, it was not considered as a possible counterpart of the source 3EG J1736-2908,…

2004 Astronomy and Astrophysics
INTEGRAL 12
Scientific objectives and selection of targets for the SMART-1 Infrared Spectrometer (SIR)
DOI: 10.1016/j.pss.2004.09.002 Bibcode: 2004P&SS...52.1261B

Keller, H. U.; Hiesinger, H.; Mall, U. +3 more

The European SMART-1 mission to the Moon, primarily a testbed for innovative technologies, was launched in September 2003 and will reach the Moon in 2005. On board are several scientific instruments, including the point-spectrometer SMART-1 Infrared Spectrometer (SIR). Taking into account the capabilities of the SMART-1 mission and the SIR instrum…

2004 Planetary and Space Science
SMART-1 11