Search Publications

Young Stellar Populations around SN 1987A
DOI: 10.1086/309212 Bibcode: 2000ApJ...539..197P

Kirshner, Robert P.; Panagia, Nino; Romaniello, Martino +1 more

We present the first results of a study of the stellar population in a region of 30 pc radius around SN 1987A, based on an analysis of multiband Hubble Space Telescope (HST) WFPC2 images. The effective temperature, radius and, possibly, reddening of each star were determined by fitting the measured broadband magnitudes to the ones calculated with …

2000 The Astrophysical Journal
eHST 68
The Host Galaxy of the Lensed Quasar Q0957+561
DOI: 10.1086/309517 Bibcode: 2000ApJ...542...74K

Peng, C. Y.; Keeton, C. R.; Kochanek, C. S. +6 more

Infrared images of the Q0957+561 gravitational lens obtained with the Hubble Space Telescope show two large (~5") lensed images of the zs=1.41 quasar host galaxy. Parts of the host galaxy are doubly imaged, like the quasar, while other parts are quadruply imaged. The distortions of the host galaxy offer the best probe yet of the global …

2000 The Astrophysical Journal
eHST 68
Binary Star Differential Photometry Using the Adaptive Optics System at Mount Wilson Observatory
DOI: 10.1086/301338 Bibcode: 2000AJ....119.2403T

Bagnuolo, William G., Jr.; Mason, Brian D.; ten Brummelaar, Theo +4 more

We present photometric and astrometric results for 36 binary systems observed with the natural guide star adaptive optics system of the Mount Wilson Institute on the 100 inch (2.5 m) Hooker Telescope. The measurements consist of differential photometry in U, B, V, R, and I filters along with astrometry of the relative positions of system component…

2000 The Astronomical Journal
Hipparcos 67
Far infrared mapping of the gas cooling along the L1448 outflow
Bibcode: 2000A&A...360..297N

Codella, C.; Benedettini, M.; Lorenzetti, D. +4 more

The molecular outflows associated with the two Class 0 sources L1448-mm and L1448-IRS3 have been mapped with the spectrometers on board the ISO satellite allowing to study in detail the physical and chemical structure of the shocked gas. The far infrared cooling is mainly due to the emission from pure rotational lines of CO, H2O and H

2000 Astronomy and Astrophysics
ISO 67
Multi-colour PL-relations of Cepheids in the bt HIPPARCOS catalogue and the distance to the LMC
DOI: 10.48550/arXiv.astro-ph/0002325 Bibcode: 2000A&A...356..849G

Groenewegen, M. A. T.; Oudmaijer, R. D.

We analyse a sample of 236 Cepheids from the hipparcos catalog, using the method of ``reduced parallaxes'' in V, I, K and the reddening-free ``Wesenheit-index''. We compare our sample to those considered by Feast & Catchpole (1997) and Lanoix et al. (1999), and argue that our sample is the most carefully selected one with respect to completene…

2000 Astronomy and Astrophysics
Hipparcos 67
Non-LTE analysis of neutral magnesium in cool stars
DOI: 10.48550/arXiv.astro-ph/0011289 Bibcode: 2000A&A...362.1077Z

Zhao, G.; Gehren, T.

Calculations of the statistical equilibrium of magnesium in the solar photosphere have shown that NLTE populations hardly affect Mg line formation in the Sun. However, in metal-poor dwarfs and giants the influence of electron collisions is reduced, and the ultraviolet radiation field, enhanced due to reduced background line opacity, results in mor…

2000 Astronomy and Astrophysics
Hipparcos 67
LINER/HII ``Transition'' Nuclei and the Nature of NGC 4569
DOI: 10.1086/316583 Bibcode: 2000PASP..112..753B

Shields, Joseph C.; Barth, Aaron J.

Motivated by the discovery of young, massive stars in the nuclei of some LINER/H II ``transition'' nuclei such as NGC 4569, we have computed photoionization models to determine whether some of these objects may be powered solely by young star clusters rather than by accretion-powered active nuclei. The models were calculated with the photoionizati…

2000 Publications of the Astronomical Society of the Pacific
eHST 67
On the Constancy of the Solar Diameter
DOI: 10.1086/317157 Bibcode: 2000ApJ...543.1007E

Kuhn, J. R.; Bush, R. I.; Emilio, M. +1 more

Why does the solar luminosity vary and could it change on human timescales by enough to affect terrestrial climate? As important as these questions are, we lack answers because we do not understand the physical mechanisms responsible for the solar irradiance cycle. Progress here depends on discovering how changes in the solar interior affect energ…

2000 The Astrophysical Journal
SOHO 66
Development of Coronal Mass Ejections: Radio Shock Signatures
DOI: 10.1086/312421 Bibcode: 2000ApJ...528L..49M

Vourlidas, Angelos; Howard, Russel; Pick, Monique +1 more

We present observational imaging evidence for the existence of metric radio bursts closely associated with the front edge of coronal mass ejections (CMEs). These radio bursts drift in frequency similarly to type II bursts. They are weak and usually go undetected on spectrograph data. We find the same measured projected velocity for the displacemen…

2000 The Astrophysical Journal
SOHO 66
The European Large Area ISO Survey - III. 90-µm extragalactic source counts
DOI: 10.1046/j.1365-8711.2000.03914.x Bibcode: 2000MNRAS.319.1169E

Genzel, R.; Danese, L.; Puget, J. -L. +17 more

We present results and source counts at 90µm extracted from the preliminary analysis of the European Large Area ISO Survey (ELAIS). The survey covered about 12deg2 of the sky in four main areas and was carried out with the ISOPHOT instrument onboard the Infrared Space Observatory (ISO). The survey is at least an order of magnitude…

2000 Monthly Notices of the Royal Astronomical Society
ISO 66