Search Publications

Kinematic Substructure of Halo Stars from HIPPARCOS Observations
DOI: 10.1086/311209 Bibcode: 1998ApJ...495L...1C

Chen, B.

With highly accurate parallaxes and proper motions observed by HIPPARCOS, we discuss the distributions of velocities and metallicities for a sample of stars selected from the Lowell Proper Motion Catalog. Cluster analysis is used to search for natural groups in the sample and display them graphically. Data presented in this Letter support the pict…

1998 The Astrophysical Journal
Hipparcos 11
The Cassini Ion Mass Spectrometer: Performance Metrics and Techniques
DOI: 10.1029/GM102p0209 Bibcode: 1998GMS...102..209N

McComas, D. J.; Young, D. T.; Goldstein, R. +7 more

The Cassini Plasma Spectrometer (CAPS) Ion Mass Spectrometer (IMS) uses a unique electric field configuration coupled with precise sub-nanosecond timing to produce a high mass-resolution plasma analyzer with both broad energy and mass ranges. The IMS maintains a spectrographic mass resolution (m/Δm) of ≥50 over a mass range of 1 to 40amu for singl…

1998 Geophysical Monograph Series
Cassini 11
Synoptic measurements of Martian winds using the Hubble Space Telescope
DOI: 10.1029/98GL50358 Bibcode: 1998GeoRL..25..611M

Crisp, David; Bell, James F., III; Mischna, Michael A. +1 more

We used the Hubble Space Telescope to make wind speed and wind direction measurements of the Martian atmosphere during early northern summer (Ls=97°). Our strategy utilized a series of near-UV images with optimal temporal sampling to track observable cloud features and to determine the direction and speed of cloud motion. Several techni…

1998 Geophysical Research Letters
eHST 11
Ulysses and WIND particle observations of the November 1997 solar events
DOI: 10.1029/98GL52667 Bibcode: 1998GeoRL..25.3469L

Lario, D.; Balogh, A.; Maksimovic, M. +5 more

The episode of intense solar activity on 4 and 6 November 1997 resulted in large and extended particle events observed by the Ulysses and WIND spacecraft. Ulysses was at a heliocentric distance of 5.34 AU, very close to the solar equator and 100° west in heliolongitude from earth. WIND was near the earth at 0.99 AU from the Sun and in the ecliptic…

1998 Geophysical Research Letters
Ulysses 11
PAH's and Crystalline Silicates in Planetary Nebulae
DOI: 10.1023/A:1001532209453 Bibcode: 1998Ap&SS.255..507B

Beintema, D. A.

An overview is given of the PAH and crystalline silicate emissions seen in the SWS guaranteed-time programme on planetary nebulae. Of the 9 objects on which good continuum measurements were obtained above 29 µm, 7 show evidence of olivine emission at 33.5 µm. PAH emission is seen in 5 of these objects, 3 objects show both PAH's and olivines. The p…

1998 Astrophysics and Space Science
ISO 11
The art of fitting p-mode spectra. II. Leakage and noise covariance matrices
DOI: 10.1051/aas:1998440 Bibcode: 1998A&AS..132..121A

Appourchaux, T.; Gizon, L.; Rabello-Soares, M. -C.

In Part I we have developed a theory for fitting p-mode Fourier spectra assuming that these spectra have a multi-normal distribution. We showed, using Monte-Carlo simulations, how one can obtain p-mode parameters using ``Maximum Likelihood Estimators". In this article, hereafter Part II, we show how to use the theory developed in Part I for fittin…

1998 Astronomy and Astrophysics Supplement Series
SOHO 11
Molecules in AGB Stars Observed with ISO
DOI: 10.1023/A:1001535723681 Bibcode: 1998Ap&SS.255..303C

Cernicharo, J.

I present in this review the recent results obtained with ISO concerning gas phase molecules in evolved stars. The near, medium and far-infrared spectrum of C-rich and O-rich stars can provide a very important information on the molecular content of these objects. Detailed models for the envelopes of AGB stars are also presented. I also report the…

1998 Astrophysics and Space Science
ISO 11
F, G and K stars in the ROSAT all-sky survey. I. Photometry
DOI: 10.1051/aas:1998431 Bibcode: 1998A&AS..131..197M

Pasquini, L.; Krautter, J.; Cutispoto, G. +2 more

We present accurate BV(RI)_c photometry for a sample of F, G and K stars detected in selected areas of the ROSAT all-sky survey (RASS). We have used the photometry, in addition to low-resolution spectroscopy, to estimate spectral classifications, distances and X-ray luminosities. The log (L_X / L_V) in the sample lies below -2. Although the sample…

1998 Astronomy and Astrophysics Supplement Series
Exosat 11
ISO Observations of Wolf-Rayet Dust Shells
DOI: 10.1023/A:1001188902783 Bibcode: 1998Ap&SS.255..169W

Morris, P. W.; van der Hucht, K. A.; Williams, P. M.

Observations of circumstellar dust clouds of Wolf-Rayet stars made with the Short Wavelength Spectrometer on ISO reveal a subtle variety of spectral energy distributions not evident from ground-based observations. The modelling of these using the radiative transfer code "Dusty" by Ivezić, Nenkova & Elitzur is reported. The results are used to …

1998 Astrophysics and Space Science
ISO 11
The Calibration of the Hubble Space Telescope Kuiper Belt Object Search: Setting the Record Straight
DOI: 10.1086/311515 Bibcode: 1998ApJ...503L..89C

Stern, S. Alan; Levison, Harold F.; Tamblyn, Peter +2 more

The limiting magnitude of the Hubble Space Telescope (HST) data set used by Cochran and coworkers in 1995 to detect small objects in the Kuiper belt is reevaluated, and the methods used are described in detail. It is shown, by implanting artificial objects in the original HST images and rereducing the images using our original algorithm, that the …

1998 The Astrophysical Journal
eHST 11