Search Publications

Dwarf spheroidal galaxies in the M81 group imaged with WFPC2
DOI: 10.48550/arXiv.astro-ph/0010146 Bibcode: 2000A&A...363..117K

Sarajedini, A.; Dolphin, A. E.; Grebel, E. K. +7 more

We obtained HST/WFPC2 images of the dwarf spheroidal (dSph) galaxies K61, K63, K64, DDO78, BK6N, and kk77 in the M81 group. Our color-magnitude diagrams show red giant branches with tips (TRGB) falling within the range of I = [23.8 -24.0] mag. The derived true distance moduli (DM) of the 6 dSphs ranging from 27.71 to 27.93 mag are consistent with …

2000 Astronomy and Astrophysics
eHST 54
Rossby waves on the Sun as revealed by solar `hills'
DOI: 10.1038/35014530 Bibcode: 2000Natur.405..544K

Kuhn, J. R.; Bush, R. I.; Scherrer, P. +1 more

It is a long-standing puzzle that the Sun's photosphere-its visible surface-rotates differentially, with the equatorial regions rotating faster than the poles. It has been suggested that waves analogous to terrestrial Rossby waves, and known as r-mode oscillations, could explain the Sun's differential rotation: Rossby waves are seen in the oceans …

2000 Nature
SOHO 54
The Hubble Space Telescope Quasar Absorption Line Key Project. XV. Milky Way Absorption Lines
DOI: 10.1086/313420 Bibcode: 2000ApJS..129..563S

Schneider, Donald P.; Savage, Blair D.; Sargent, W. L. W. +10 more

This paper presents the results of an analysis of the Milky Way absorption lines found in the Hubble Space Telescope (HST) Quasar Absorption Line Key Project database for 83 QSOs observed with the Faint Object Spectrograph G190H and G270H gratings, of which 16 QSOs are also observed with the G130H grating. The HST Key Project observations are supp…

2000 The Astrophysical Journal Supplement Series
eHST 53
Pluto's Non-isothermal Surface
DOI: 10.1006/icar.2000.6441 Bibcode: 2000Icar..147..220L

Lellouch, E.; Crovisier, J.; Coustenis, A. +4 more

We report on repeated far-infrared photometric observations of the Pluto-Charon system conducted in 1997 with the Infrared Space Observatory (ISO). These observations have led to the first detection of the system at 150 and 200 µm and to the first clear detection of its thermal lightcurve at 60 µm (and more marginally at 100 µm).…

2000 Icarus
ISO 53
Rings in the Planetesimal Disk of β Pictoris
DOI: 10.1086/312494 Bibcode: 2000ApJ...530L.133K

Schultz, A.; Kalas, P.; Larwood, J. +1 more

The nearby main-sequence star β Pictoris is surrounded by an edge-on disk of dust produced by the collisional erosion of larger planetesimals. Here we report the discovery of substructure within the northeast extension of the disk midplane that may represent an asymmetric ring system around β Pic. We present a dynamical model showing that a close …

2000 The Astrophysical Journal
eHST 53
The Extreme-Ultraviolet Solar Irradiance Spectrum Observed with the Coronal Diagnostic Spectrometer (CDS) on SOHO
DOI: 10.1086/308966 Bibcode: 2000ApJ...536..959B

Brekke, P.; Thompson, W. T.; Woods, T. N. +1 more

We present a calibrated solar EUV irradiance spectrum in the ranges 307-380 Å and 515-632 Å. The ``Sun as a star'' spectrum was recorded by the Coronal Diagnostic Spectrometer (CDS) on SOHO on 1997 May 15 using the normal incidence spectrometer (NIS) with a spectral resolution between 0.3 and 0.6 Å. The relatively high spectral resolution allows t…

2000 The Astrophysical Journal
SOHO 53
Analysis of a Solar Active Region Extreme-Ultraviolet Spectrum from SERTS-97
DOI: 10.1086/317153 Bibcode: 2000ApJ...543.1016B

Landi, Enrico; Brosius, Jeffrey W.; Thomas, Roger J. +1 more

Goddard Space Flight Center's Solar EUV Research Telescope and Spectrograph was flown on 1997 November 18, carrying an intensified CCD detector and a multilayer-coated toroidal diffraction grating with enhanced sensitivity over that of a standard gold-coated grating throughout the instrument's 299-353 Å spectral bandpass. Spectra and spectroheliog…

2000 The Astrophysical Journal
SOHO 53
Adding More Mysteries to the DA White Dwarf GD 394
DOI: 10.1086/309079 Bibcode: 2000ApJ...537..977D

Vennes, Stéphane; Christian, Damian J.; Chayer, Pierre +2 more

We present spectroscopic and timing analyses of the hot DA white dwarf GD 394 showing abundance inhomogeneities across its surface. Lick Hamilton echelle, International Ultraviolet Explorer (IUE), HST GHRS, and Hopkins Ultraviolet Telescope (HUT) spectra show dominant Si III and Si IV features, while Extreme Ultraviolet Explorer (EUVE) spectra sho…

2000 The Astrophysical Journal
IUE eHST 53
ISO observations of a sample of Compact Steep Spectrum and GHz Peaked Spectrum radio galaxies
DOI: 10.48550/arXiv.astro-ph/0005035 Bibcode: 2000A&A...358..499F

Pozzi, F.; Bremer, M.; Dallacasa, D. +13 more

We present results from observations obtained with ISOPHOT, on board the ISO satellite, of a representative sample of seventeen CSS/GPS radio galaxies and of a control sample of sixteen extended radio galaxies spanning similar ranges in redshift (0.2 <= z <= 0.8) and radio luminosity (P_{2.7 GHz} >= 1026 W/Hz). The observations…

2000 Astronomy and Astrophysics
ISO 53
The coupling of solar convection and rotation - (Invited Review)
DOI: 10.1023/A:1005260527450 Bibcode: 2000SoPh..192...59M

Miesch, Mark S.

In recent years, helioseismology has provided an unprecedented look at the dynamics of the solar interior. These new insights have been accompanied by tremendous advances in high-performance computing technology, prompting increasingly sophisticated and realistic numerical models of solar convection. Among the most important helioseismic constrain…

2000 Solar Physics
SOHO 53