Search Publications

Interpretation of the UV spectrum of some stars with little reddening
DOI: 10.1016/S1384-1076(00)00030-0 Bibcode: 2000NewA....5..285Z

Zagury, Frédéric

The UV spectrum of a few reddened stars will be decomposed into two terms. One is the direct starlight, F ★,λ0 eλ, which is the product of the flux of the star corrected for interstellar extinction, F★, λ0, and of the extinction e - τλ. The second is starlig…

2000 New Astronomy
IUE 12
Orbital period variation in close binaries from radial velocity data and magnetic activity cycles. I. AR Lacertae: The test case
Bibcode: 2000A&A...356..267F

Lanza, A. F.; Frasca, A.

We check the possibility of detecting orbital period changes in non-eclipsing close binaries by means of spectroscopic orbit determinations. In order to test our method, we selected the eclipsing binary AR Lacertae for which the spectroscopically determined epochs of superior conjuctions can be compared with those provided by the light minima phot…

2000 Astronomy and Astrophysics
IUE 12
Global Solar Corona Revealed by Time Series Observations
DOI: 10.1086/309110 Bibcode: 2000ApJ...538..415L

Raymond, J. C.; Li, Jing; Kuhn, J. +2 more

Time series observations at UV (Extreme Ultraviolet Imaging Telescope/Solar and Heliospheric Observatory) and X-ray (Soft X-Ray Telescope/Yohkoh) wavelengths reveal properties of the global solar corona that are not easily identified in a single image. A median-filtering technique that rejects features varying with time is used to isolate backgrou…

2000 The Astrophysical Journal
SOHO 12
Comparing Tycho-2 Astrometry with UCAC1
DOI: 10.1086/301474 Bibcode: 2000AJ....120.1148Z

Zacharias, N.; Urban, S. E.; Zacharias, M. I. +1 more

The Tycho-2 Catalogue, released in February 2000, is based on the ESA Hipparcos space mission data and various ground-based catalogs for proper motions. An external comparison of the Tycho-2 astrometry is presented here using the first US Naval Observatory CCD Astrograph Catalog (UCAC1). The UCAC1 data were obtained from observations performed at …

2000 The Astronomical Journal
Hipparcos 12
Determination of the abundance of aluminum in the solar wind with SOHO/CELIAS/MTOF
DOI: 10.1029/1999JA005085 Bibcode: 2000JGR...10512659B

Bochsler, Peter; Wurz, Peter; Weygand, James M. +2 more

The Al/Mg abundance ratio provides an excellent test case for investigating possible fractionation processes among low First Ionization Potential (FIP) elements in the solar wind. Al and Mg are refractory elements; their abundance ratio has been well determined in solar system materials and inferences for the abundance ratio in the solar atmospher…

2000 Journal of Geophysical Research
SOHO 12
A combined approach for object detection and deconvolution
DOI: 10.1051/aas:2000293 Bibcode: 2000A&AS..147..139S

Valtchanov, I.; Starck, J. -L.; Bijaoui, A. +1 more

The Multiscale Vision Model is a recent object detection method, based on the wavelet transform. It allows us to extract all objects contained in an image, whatever their size or their shape. From each extracted object, information concerning flux or shape can easily be determined. We show that such an approach can be combined with deconvolution, …

2000 Astronomy and Astrophysics Supplement Series
ISO 12
The bright 175 mu m knots of the Andromeda galaxy
DOI: 10.48550/arXiv.astro-ph/0009494 Bibcode: 2000A&A...363..917S

Lemke, D.; Haas, M.; Schmidtobreick, L.

Discrete far-infrared (FIR) sources of M 31 are identified in the ISO 175 mu m map and characterized via their FIR colours, luminosities and masses in order to reveal the nature of these knots. With our spatial resolution of 300 pc at M 31's distance, the FIR knots are clearly seen as extended objects with a mean size of about 800 pc. Since this a…

2000 Astronomy and Astrophysics
ISO 12
Light-Element Abundance Patterns in the Orion Association. I.Hubble Space Telescope Observations of Boron in G Dwarfs
DOI: 10.1086/317139 Bibcode: 2000ApJ...543..850C

Cunha, Katia; Smith, Verne V.; Lambert, David L. +1 more

The boron abundances for two young solar-type members of the Orion association, BD -6°1250 and HD 294297, are derived from Hubble Space Telescope STIS spectra of the B I transition at 2496.771 Å. The best-fit boron abundances for the target stars are 0.13 and 0.44 dex lower than the solar meteoritic value of logɛ(B)=2.78. An anticorrelation of bor…

2000 The Astrophysical Journal
eHST 12
In-Flight Determination of the Plate Scale of the Extreme-Ultraviolet Imaging Telescope
DOI: 10.1086/312471 Bibcode: 2000ApJ...529L.115A

Auchère, F.; Artzner, G.; DeForest, C. E.

Using simultaneous observations of the Michelson Doppler Imager and Extreme-Ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory spacecraft, we determined in flight the plate scale of the EIT. We found a value of 2.629"+/-0.001" pixel-1, in fair agreement with the 2.627"+/-0.001" pixel-1 value d…

2000 The Astrophysical Journal
SOHO 12
Hubble Space Telescope Observations of M Subdwarfs
DOI: 10.1086/316558 Bibcode: 2000PASP..112..610G

Gizis, John E.; Reid, I. Neill

We present the results of a Hubble Space Telescope snapshot program to search for very low mass stellar companions to nearby M subdwarfs. None of our nine targetted metal-poor primaries has companions more massive than the hydrogen burning limit, implying that the halo binary fraction is equal to or less than the Galactic disk binary fraction belo…

2000 Publications of the Astronomical Society of the Pacific
eHST 12