Search Publications

Jet-induced Emission-Line Nebulosity and Star Formation in the High-Redshift Radio Galaxy 4C 41.17
DOI: 10.1086/309343 Bibcode: 2000ApJ...540..678B

Dey, Arjun; Dopita, Michael A.; Sutherland, Ralph S. +3 more

The high-redshift radio galaxy 4C 41.17 has been shown in earlier work to consist of a powerful radio source in which there is strong evidence for jet-induced star formation along the radio axis. We argue that nuclear photoionization is not responsible for the excitation of the emission line clouds, and we construct a jet-cloud interaction model t…

2000 The Astrophysical Journal
eHST 172
Kinematics of Metal-poor Stars in the Galaxy. II. Proper Motions for a Large Nonkinematically Selected Sample
DOI: 10.1086/301410 Bibcode: 2000AJ....119.2866B

Beers, Timothy C.; Rossi, Silvia; Platais, Imants +4 more

We present a revised catalog of 2106 Galactic stars, selected without kinematic bias and with available radial velocities, distance estimates, and metal abundances in the range -4.0<=[Fe/H]<=0.0. This update of the 1995 Beers & Sommer-Larsen catalog includes newly derived homogeneous photometric distance estimates, revised radial velocit…

2000 The Astronomical Journal
Hipparcos 172
Basic Principles of Solar Acoustic Holography - (Invited Review)
DOI: 10.1023/A:1005227200911 Bibcode: 2000SoPh..192..261L

Braun, D. C.; Lindsey, C.

We summarize the basic principles of holographic seismic imaging of the solar interior, drawing on familiar principles in optics and parallels with standard optical holography. Computational seismic holography is accomplished by the phase-coherent wave-mechanical reconstruction of the p-mode acoustic field into the solar interior based on heliosei…

2000 Solar Physics
SOHO 171
Modelling irradiance variations from the surface distribution of the solar magnetic field
Bibcode: 2000A&A...353..380F

Solanki, S. K.; Unruh, Y. C.; Fligge, M.

An important question in solar physics is to what extent solar surface magnetism affects the solar irradiance. Previous attempts to answer this question have employed proxies of the magnetic field to reconstruct the irradiance and compare it with observations. Here we present the first model calculations of solar irradiance variations based on var…

2000 Astronomy and Astrophysics
SOHO 171
Exploring the brown dwarf desert with Hipparcos
Bibcode: 2000A&A...355..581H

Queloz, D.; Arenou, F.; Udry, S. +2 more

The orbital elements of 11 spectroscopic binaries with brown dwarf candidates (M2 sin i between 0.01 and 0.08 Msun) are combined with the Hipparcos observations in order to derive astrometric orbits. Estimations of the masses of the secondary components are thus calculated. It appears that 5 secondary masses are more than 2 s…

2000 Astronomy and Astrophysics
Hipparcos 166
Identification of a Nearby Stellar Association in theHipparcos Catalog: Implications for Recent, Local Star Formation
DOI: 10.1086/308897 Bibcode: 2000ApJ...535..959Z

Zuckerman, B.; Webb, R. A.

The TW Hydrae Association (~55 pc from Earth) is the nearest known region of recent star formation. Based primarily on the Hipparcos catalog, we have identified a group of nine or 10 comoving star systems at a common distance (~45 pc) from Earth that appear to comprise another, somewhat older association (``the Tucanae Association''). Together wit…

2000 The Astrophysical Journal
Hipparcos 162
The Hubble Space Telescope Survey of BL Lacertae Objects. I. Surface Brightness Profiles, Magnitudes, and Radii of Host Galaxies
DOI: 10.1086/308618 Bibcode: 2000ApJ...532..740S

Urry, C. Megan; Scarpa, Riccardo; Treves, Aldo +2 more

We report on a large Hubble Space Telescope imaging survey of BL Lac objects, at spatial resolution >~10 times better than previous ground-based surveys. We focus on data reduction and analysis, describing the procedures used to model the host galaxy surface brightness radial profiles. A total of 69 host galaxies were resolved out of 110 object…

2000 The Astrophysical Journal
eHST 161
Models for Old, Metal-Poor Stars with Enhanced α-Element Abundances. II. Their Implications for the Ages of the Galaxy's Globular Clusters and Field Halo Stars
DOI: 10.1086/313404 Bibcode: 2000ApJS..129..315V

VandenBerg, Don A.

The ages of globular clusters (GCs) and post-turnoff field stars in the Galactic halo are derived using new stellar evolutionary models that explicitly take into account the observed abundances of the α-elements. Whereas the distances of the field subgiants considered in this study are based on Hipparcos parallax measurements, theoretical zero-age…

2000 The Astrophysical Journal Supplement Series
Hipparcos 161
Resolved Spectroscopy of the Narrow-Line Region in NGC 1068: Kinematics of the Ionized Gas
DOI: 10.1086/312581 Bibcode: 2000ApJ...532L.101C

Crenshaw, D. Michael; Kraemer, Steven B.

We have determined the radial velocities of the [O III]-emitting gas in the inner narrow-line region of the Seyfert 2 galaxy NGC 1068, along a slit at position angle 202 deg, from STIS observations at a spatial resolution of 0.1" and a spectral resolving power of λ/Δλ~1000. We use these data to investigate the kinematics of the narrow-line region …

2000 The Astrophysical Journal
eHST 160
2.5-11 micron spectroscopy and imaging of AGNs. Implication for unification schemes
DOI: 10.48550/arXiv.astro-ph/0003298 Bibcode: 2000A&A...357..839C

Altieri, B.; Clavel, J.; Metcalfe, L. +6 more

We present low resolution spectrophotometric and imaging ISO observations of a sample of 57 AGNs and one non-active SB galaxy over the 2.5-11 mu m range. The sample is about equally divided into type I (<= 1.5; 28 sources) and type II (> 1.5; 29 sources) objects. The mid-IR (MIR) spectra of type I (Sf1) and type II (Sf2) objects are statisti…

2000 Astronomy and Astrophysics
ISO 158