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Cumulants and symmetries in a trivariate normal mixture. A qualitative study of the local velocity distribution
DOI: 10.1051/0004-6361:20041144 Bibcode: 2004A&A...427..131C

Cubarsi, R.; Alcobé, S.

An alternative parameterization of a trivariate normal mixture for the stellar velocity distribution provides a set of constraint equations between global cumulants that are used to estimate characteristic constants of the mixture and population parameters. Under particular distribution symmetries these relationships become simpler and easy to eva…

2004 Astronomy and Astrophysics
Hipparcos 15
Discovery of a new INTEGRAL source: IGR J19140+0951
DOI: 10.1051/0004-6361:200400021 Bibcode: 2004A&A...423L..17H

Rodriguez, J.; Henri, G.; Petrucci, P. O. +5 more

IGR J19140+0951 (formerly known as IGR J19140+098) was discovered with the INTEGRAL satellite in March 2003. We report the details of the discovery, using an improved position for the analysis. We have performed a simultaneous study of the 5-100 keV JEM-X and ISGRI spectra from which we can distinguish two different states. From the results of our…

2004 Astronomy and Astrophysics
INTEGRAL 15
The Counterstreaming Instability in Dwarf Elliptical Galaxies with Off-Center Nuclei
DOI: 10.1086/383088 Bibcode: 2004ApJ...603L..25D

Debattista, Victor P.; De Rijcke, Sven

In many nucleated dwarf elliptical galaxies (dE,N's), the nucleus is offset by a significant fraction of the scale radius with respect to the center of the outer isophotes. Using a high-resolution N-body simulation, we demonstrate that the nucleus can be driven off-center by the m=1 counterstreaming instability, which is strong in flattened stella…

2004 The Astrophysical Journal
eHST 15
Wolf-Rayet stars in M33 - I. Optical spectroscopy using CFHT-MOS
DOI: 10.1111/j.1365-2966.2004.07663.x Bibcode: 2004MNRAS.350..552A

Drissen, Laurent; Crowther, Paul A.; Dessart, Luc +3 more

We have obtained spectroscopy of a large sample of Wolf-Rayet stars in M33 with the Canada-France-Hawaii Telescope Multi-Object Spectrograph (CFHT-MOS), including 26 WC stars, 15 WN stars and a WN/C star. In general, spectral types are merely refined, although the spectral type of X9 from Massey & Johnson is revised from WNL?+abs to WC4+abs, w…

2004 Monthly Notices of the Royal Astronomical Society
eHST 15
The Orbits of the Inner Neptunian Satellites from Voyager, Earth-based, and Hubble Space Telescope Observations
DOI: 10.1086/423037 Bibcode: 2004AJ....128.1412J

Jacobson, R. A.; Owen, W. M., Jr.

We present revised orbital elements for the six small Neptunian satellites discovered by Voyager 2. The elements have been determined from a fit to imaging data acquired by the Voyager 2 spacecraft and astrometric observations made at Earth-based observatories and by the Hubble Space Telescope. An assessment of the accuracy of the elements is prov…

2004 The Astronomical Journal
eHST 15
The dependence of Langmuir wave amplitudes on position in Earth's foreshock
DOI: 10.1029/2004GL019413 Bibcode: 2004GeoRL..31.7805S

Gurnett, D. A.; Balogh, A.; Pickett, J. S. +3 more

We present the first results of Langmuir wave observations in the foreshock from the Cluster WBD Plasma Wave Receiver. When the data were binned by distance to the foreshock boundary, the Langmuir wave amplitude probability distributions followed the log-normal statistics predicted by stochastic growth theory for all regions of the foreshock. The …

2004 Geophysical Research Letters
Cluster 15
Stellar activity and magnetism studied by optical interferometry
DOI: 10.1051/0004-6361:20040151 Bibcode: 2004A&A...422..193R

Jankov, S.; Kilbinger, M.; Lanz, T. +5 more

By means of numerical simulations, we investigate the ability of optical interferometry, via the fringe phase observable, to address stellar activity and magnetism. To derive abundance maps and stellar rotation axes, we use color differential interferometry which couples high angular resolution to high spectral resolution. To constrain magnetic fi…

2004 Astronomy and Astrophysics
SOHO 15
Optical and infrared spectroscopic analysis of the post-AGB star candidate IRAS 19386+0155
DOI: 10.1051/0004-6361:20035592 Bibcode: 2004A&A...422..637P

Pereira, C. B.; Lorenz-Martins, S.; Machado, M.

This work reports high-resolution spectroscopic stellar parameters and abundance analysis of the post-AGB star IRAS 19386+0155. The analysis of the high resolution spectrum shows that it has an effective temperature of Teff=6800±100 K and a surface gravity of log g = 1.4±0.2. The abundance analysis reveals IRAS 19386+0155 to be a metal-…

2004 Astronomy and Astrophysics
ISO 15
The circumstellar environment of IRAS 16293-2422. ISO-LWS and SCUBA observations
DOI: 10.1051/0004-6361:20040056 Bibcode: 2004A&A...418..607C

Griffin, M.; Saraceno, P.; Correia, J. C.

We present far-infrared (FIR) continuum observations of the deeply embedded source IRAS 16293-2422 performed with the Long Wavelength Spectrometer (LWS) on-board the Infrared Space Observatory (ISO). We also report 450 and 850 µm mapping observations done with the Submillimetre Common-User Bolometer Array (SCUBA) at the James Clerk Maxwell T…

2004 Astronomy and Astrophysics
ISO 15
Dual Flows with Supersonic Velocities in the Sunspot Transition Region
DOI: 10.1086/422838 Bibcode: 2004ApJ...612.1193B

Wilhelm, K.; Kjeldseth-Moe, O.; Brynildsen, N. +1 more

Observations of sunspot transition region lines that deviate significantly from a Gaussian shape are presented. Attention is given to ``dual flows,'' a line profile phenomenon in which two distinct velocities are observed within the same spatial resolution element. In 5 out of 12 sunspots we observe dual flows. Several emission line profiles are w…

2004 The Astrophysical Journal
SOHO 15