Search Publications

The Distribution of Nearby Stars in Velocity Space Inferred from HIPPARCOS Data
DOI: 10.1086/300364 Bibcode: 1998AJ....115.2384D

Dehnen, Walter

The velocity distribution f(v) of nearby stars is estimated, via a maximum likelihood algorithm, from the positions and tangential velocities of a kinematically unbiased sample of 14,369 stars observed by the Hipparcos satellite. The distribution f shows rich structure in the radial and azimuthal motions, v_R and v_phi, but not in the vertical vel…

1998 The Astronomical Journal
Hipparcos 361
The Sun's total irradiance: Cycles, trends and related climate change uncertainties since 1976
DOI: 10.1029/1998GL900157 Bibcode: 1998GeoRL..25.4377F

Fröhlich, Claus; Lean, Judith

A composite record of the Sun's total irradiance compiled from measurements made by five independent space-based radiometers since 1978 exhibits a prominent 11-year cycle with similar levels during 1986 and 1996, the two most recent minimum epochs of solar activity. This finding contradicts recent assertions of a 0.04% irradiance increase from the…

1998 Geophysical Research Letters
SOHO 359
New models of Jupiter's magnetic field constrained by the Io flux tube footprint
DOI: 10.1029/97JA03726 Bibcode: 1998JGR...10311929C

Connerney, J. E. P.; Satoh, T.; Acuña, M. H. +1 more

Spherical harmonic models of the planetary magnetic field of Jupiter are obtained from in situ magnetic field measurements and remote observations of the position of the foot of the Io flux tube in Jupiter's ionosphere. The Io flux tube (IFT) footprint locates the ionospheric footprint of field lines traced from Io's orbital radial distance in the…

1998 Journal of Geophysical Research
eHST 341
Detailed Mass Map of CL 0024+1654 from Strong Lensing
DOI: 10.1086/311314 Bibcode: 1998ApJ...498L.107T

Tyson, J. Anthony; Kochanski, Greg P.; Dell'Antonio, Ian P.

We construct a high-resolution mass map of the z=0.39 cluster 0024+1654, based on a parametric inversion of the associated gravitational lens. The lens creates eight well-resolved subimages of a background galaxy, seen in deep imaging with the Hubble Space Telescope.1 Excluding mass concentrations centered on visible galaxies, more than 98% of the…

1998 The Astrophysical Journal
eHST 335
Steps toward interstellar silicate mineralogy. IV. The crystalline revolution
Bibcode: 1998A&A...339..904J

Waters, L. B. F. M.; Mutschke, H.; Henning, Th. +3 more

Mid- and far-infrared spectra gained by the Short Wavelength Spectrometer (SWS) of the Infrared Space Observatory (ISO) satellite have provided striking evidence for the presence of crystalline silicates in comets, circumstellar envelopes around young stars and, most of all, evolved stars and planetary nebulae. Since optical properties of astrophy…

1998 Astronomy and Astrophysics
ISO 334
The Age of Globular Clusters in Light of Hipparcos: Resolving the Age Problem?
DOI: 10.1086/305201 Bibcode: 1998ApJ...494...96C

Chaboyer, Brian; Demarque, P.; Kernan, Peter J. +1 more

We review five independent techniques that are used to set the distance scale to globular clusters, including subdwarf main-sequence fitting utilizing the recent Hipparcos parallax catalog. These data together all indicate that globular clusters are farther away than previously believed, implying a reduction in age estimates. We now adopt a best-f…

1998 The Astrophysical Journal
Hipparcos 322
The spectrum of the young star HD 100546 observed with the Infrared Space Observatory
Bibcode: 1998A&A...332L..25M

Waters, L. B. F. M.; Vandenbussche, B.; Waelkens, C. +3 more

It is generally assumed that planets form in the dusty disks that surround young stars (Beckwith & Sargent 1996). The Infrared Space Observatory (Kessler et al. 1996) now enables us to determine the characteristics of these disks with unprecedented spectral resolution and signal-to-noise. We present here ISO spectra of the disk that surrounds …

1998 Astronomy and Astrophysics
ISO 320
High-z Lyalpha Emitters. I. A Blank-Field Search for Objects near Redshift Z = 3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA 22
DOI: 10.1086/300309 Bibcode: 1998AJ....115.1319C

Cowie, Lennox L.; Hu, Esther M.

We present deep narrowband (lambda = 5390 Å, Deltalambda = 77 Å) and multicolor observations of the Hubble Deep Field and the Hawaii Deep Field SSA 22 obtained with the LRIS instrument at the 10 m Keck II Telescope. It is shown that there is a substantial population of galaxies at z ~ 3.4 that can be selected by Lyalpha emission. Comparison with c…

1998 The Astronomical Journal
eHST 316
The Nature and Evolution of Ultraluminous Infrared Galaxies:A Mid-Infrared Spectroscopic Survey
DOI: 10.1086/311614 Bibcode: 1998ApJ...505L.103L

Lutz, D.; Genzel, R.; Rigopoulou, D. +2 more

We report the first results of a low-resolution mid-infrared spectroscopic survey of an unbiased, far-infrared-selected sample of 60 ultraluminous infrared galaxies (ULIRGs) (LIR>1012 Lsolar) using ISOPHOT-S on board the Infrared Space Observatory (ISO). We use the ratio of the 7.7 µm ``polycyclic aromatic…

1998 The Astrophysical Journal
ISO 305
The Hubble Space Telescope Key Project on the Extragalactic Distance Scale. XIII. The Metallicity Dependence of the Cepheid Distance Scale
DOI: 10.1086/305538 Bibcode: 1998ApJ...498..181K

Illingworth, Garth D.; Huchra, John P.; Madore, Barry F. +22 more

Uncertainty in the metal-abundance dependence of the Cepheid variable period-luminosity (PL) relation remains one of the outstanding sources of systematic error in the extragalactic distance scale and in the Hubble constant. To test for such a metallicity dependence, we have used the Wide Field Planetary Camera 2 (WFPC2) on the Hubble Space Telesc…

1998 The Astrophysical Journal
eHST 297