Search Publications

Another View of the EIT Wave Phenomenon
DOI: 10.1086/317777 Bibcode: 2000ApJ...545..512D

Delannée, C.

This paper investigates three different EIT waves. The events occurred on 1997 November 3 at 10:31 UT, on 1998 January 27 at 22:19 UT, and on 1998 June 13 at 15:23 UT and were observed with EIT on board the Solar and Heliospheric Observatory (SOHO) using the 195 Å filter that contains an Fe XII line. The three events show the following similar str…

2000 The Astrophysical Journal
SOHO 148
Photometric Redshifts and Selection of High-Redshift Galaxies in the NTT and Hubble Deep Fields
DOI: 10.1086/316803 Bibcode: 2000AJ....120.2206F

Fontana, Adriano; Saracco, Paolo; Moorwood, Alan +5 more

We present and compare in this paper new photometric redshift catalogs of the galaxies in three public fields: the NTT Deep Field, the HDF-N, and the HDF-S. In the case of the NTT Deep Field, we present here a new photometric catalog, obtained by combining the existing BVrI and JKs with new deep U observations acquired with NTT-SUSI2, and which in…

2000 The Astronomical Journal
eHST 148
The First US Naval Observatory CCD Astrograph Catalog
DOI: 10.1086/301563 Bibcode: 2000AJ....120.2131Z

Zacharias, N.; Urban, S. E.; Wycoff, G. L. +9 more

The USNO CCD Astrograph (UCA) started an astrometric survey in 1998 February at Cerro Tololo, Chile. This first, preliminary catalog (UCAC1) includes data taken up to 1999 November with about 80% of the Southern Hemisphere covered. Observing continues, and full sky coverage is expected by mid-2003 after moving the instrument to a Northern Hemisphe…

2000 The Astronomical Journal
Hipparcos 147
A global MHD solar wind model with WKB Alfvén waves: Comparison with Ulysses data
DOI: 10.1029/1999JA000233 Bibcode: 2000JGR...10512675U

Goldstein, Melvyn L.; Usmanov, Arcadi V.; Besser, Bruno P. +1 more

We use a steady state global axisymmetric MHD model to reproduce quantitatively the Ulysses observations during its first fast latitude traversal in 1994-1995. In particular, we are able to account for the transformation of a surface dipole magnetic field near the Sun into the configuration observed at large heliocentric distances. The MHD equatio…

2000 Journal of Geophysical Research
Ulysses 147
The structure of the collapsing envelope around the low-mass protostar IRAS 16293-2422
Bibcode: 2000A&A...355.1129C

Ceccarelli, C.; Caux, E.; Tielens, A. G. G. M. +4 more

Using H2O, OI and SiO data, we derive the structure of the collapsing envelope around the low-mass protostar IRAS16293-2422 down to r ~ 30 AU. With an accurate model which computes self-consistently the chemical composition, thermal balance and line emission from a collapsing envelope (Ceccarelli et al. 1996), we find that IRAS16293-242…

2000 Astronomy and Astrophysics
ISO 146
Multiple shells in IRC+10216: shell properties
Bibcode: 2000A&A...359..707M

Mauron, N.; Huggins, P. J.

We report on the properties of the multiple shells in the circumstellar envelope of IRC+10216, using deep optical imaging, including data from the Hubble Space Telescope. The intensity profiles confirm the presence of thin ( ~ 0farcs5 -3'' ec), limb-brightened shells in the envelope, seen in stellar and ambient Galactic light scattered by dust. Th…

2000 Astronomy and Astrophysics
eHST 145
Slow magnetoacoustic waves in coronal loops
Bibcode: 2000A&A...362.1151N

Berghmans, D.; Nakariakov, V. M.; Verwichte, E. +1 more

A theoretical model interpreting propagating disturbances of EUV emission intensity, recently observed in coronal loops, is constructed in terms of slow magnetoacoustic waves. The model is one-dimensional and incorporates effects of nonlinearity, dissipation due to finite viscosity and thermal conduction, and gravitational stratification of plasma…

2000 Astronomy and Astrophysics
SOHO 144
The Evolution of Early-Type Galaxies in Distant Clusters. III. M/LV Ratios in the z=0.33 Cluster CL 1358+62
DOI: 10.1086/308440 Bibcode: 2000ApJ...531..184K

van Dokkum, Pieter G.; Franx, Marijn; Kelson, Daniel D. +1 more

Internal kinematics, length scales, and surface brightnesses have been determined for a large sample of 53 galaxies in the cluster Cl 1358+62 at z=0.33 from Keck spectroscopy and Hubble Space Telescope WFPC2 imaging over a 1.5 h-1x1.5 h-1 Mpc2 field of view. These data have been used to constrain the evolution of e…

2000 The Astrophysical Journal
eHST 144
Hubble Space Telescope NICMOS Images of Herbig-Haro Energy Sources: [Fe II] Jets, Binarity, and Envelope Cavities
DOI: 10.1086/301510 Bibcode: 2000AJ....120.1449R

Bally, John; Rodríguez, Luis F.; Reipurth, Bo +2 more

We have observed seven regions surrounding the driving sources of Herbig-Haro flows using the NICMOS infrared camera on board the Hubble Space Telescope. These Herbig-Haro energy sources, which power the HH 34, 47, 83, 111, 199, 300, and 454 flows, have all been previously detected in the centimeter-wavelength radio continuum. The regions were ima…

2000 The Astronomical Journal
eHST 144
Detection and Photometry of Hot Horizontal Branch Stars in the Core of M32
DOI: 10.1086/308566 Bibcode: 2000ApJ...532..308B

Ferguson, Henry C.; Brown, Thomas M.; Kimble, Randy A. +2 more

We present the deepest near-UV image of M32 to date, which for the first time resolves hot horizontal branch (HB) stars in an elliptical galaxy. Given the near-solar metallicity of M32, much larger than that of globular clusters, the existence of an extended horizontal branch is a striking example of the second parameter effect, and, most importan…

2000 The Astrophysical Journal
eHST 143