Search Publications

Laboratory investigation on the formation of unsaturated nitriles in Titan's atmosphere
DOI: 10.1016/S0032-0633(00)00018-0 Bibcode: 2000P&SS...48..447B

Kaiser, R. I.; Balucani, N.; Asvany, O. +3 more

Crossed molecular beam experiments of ground state cyano radicals, CN(X 2Σ +), with hydrocarbons acetylene (C 2H 2), ethylene (C 2H 4), methylacetylene (CH 3CCH), allene (H 2CCCH 2), dimethylacetylene (CH 3CCCH 3), and benzene (…

2000 Planetary and Space Science
Huygens 48
Local Luminosity Function at 15 Microns and Galaxy Evolution Seen by ISOCAM 15 Micron Surveys
DOI: 10.1086/309401 Bibcode: 2000ApJ...541..134X

Xu, Cong

A local luminosity function at 15 µm is derived using the bivariate (15 µm vs. 60 µm luminosity) method, based on the newly published ISOCAM LW3 band (15 µm) survey of the very deep IRAS 60 µm sample in the north ecliptic pole region (NEPR). New IRAS 60 µm fluxes are obtained using the SCANPI/SUPERSCANPI softwar…

2000 The Astrophysical Journal
ISO 48
A moving group of young stars in Carina-Vela
DOI: 10.1046/j.1365-8711.2000.03584.x Bibcode: 2000MNRAS.317..289M

Makarov, Valeri V.; Urban, Sean

Accurate two-colour photometry and proper motions of 7096 young X-ray stars in the ROSAT All-Sky Survey Bright Star Catalogue, version 1RXS, are extracted from the Tycho-2 Catalogue. The sample is dominated by red main-sequence and possibly pre-main-sequence stars. On a global proper motion convergence map, two features are very prominent: the nea…

2000 Monthly Notices of the Royal Astronomical Society
Hipparcos 48
A numerical study of the evolution of the solar wind from Ulysses to Voyager 2
DOI: 10.1029/1999JA900436 Bibcode: 2000JGR...105.2337W

Wang, C.; Richardson, J. D.; Gosling, J. T.

Voyager 2 continues to explore the outer heliosphere as Ulysses studies the latitudinal dependence of the solar wind. During the year 1991 these spacecraft were within 2° latitude and their radial separation was larger than 30 AU. This alignment presents a good opportunity to investigate the evolution of the solar wind and, in particular, the effe…

2000 Journal of Geophysical Research
Ulysses 48
ROSAT HRI catalogue of X-ray sources in the LMC region
DOI: 10.1051/aas:2000185 Bibcode: 2000A&AS..143..391S

Pietsch, W.; Haberl, F.; Sasaki, M.

All 543 pointed observations of the ROSAT High Resolution Imager (HRI) with exposure times higher than 50 s and performed between 1990 and 1998 in a field of 10°\ x 10°\ covering the Large Magellanic Cloud (LMC) were analyzed. A catalogue was produced containing 397 X-ray sources with their properties measured by the HRI. The list was cross-correl…

2000 Astronomy and Astrophysics Supplement Series
Hipparcos 48
The Evolving Morphology of the Bipolar Nebula M2-9
DOI: 10.1086/301267 Bibcode: 2000AJ....119.1339D

Corradi, R. L. M.; Balick, Bruce; Schwarz, H. E. +1 more

The planetary nebula M2-9 has drastically changed its shape since its discovery by Minkwoski. Although the outline of the nebula seems to be stationary, most of the knots and bright features (N1, N2, S1, and S2) have moved laterally from the west to the east edges of both lobes. These features and their changes have reflection, not point, symmetry…

2000 The Astronomical Journal
eHST 48
Hydrogen Lyα Absorption Predictions by Boltzmann Models of the Heliosphere
DOI: 10.1086/309541 Bibcode: 2000ApJ...542..493W

Zank, Gary P.; Wood, Brian E.; Müller, Hans-Reinhard

We use self-consistent kinetic/hydrodynamic models of the heliosphere to predict H I Lyα absorption profiles for various lines of sight through the heliosphere. These results are compared with Lyα absorption lines of six nearby stars observed by the Hubble Space Telescope. The directions of these lines of sight range from nearly upwind (36 Oph) to…

2000 The Astrophysical Journal
eHST 48
The Mass Function of Main-Sequence Stars in NGC 6397 from Near-Infrared and Optical High-Resolution Hubble Space Telescope Observations
DOI: 10.1086/308334 Bibcode: 2000ApJ...530..342D

Paresce, Francesco; De Marchi, Guido; Pulone, Luigi

We have investigated the properties of the stellar mass function in the globular cluster NGC 6397 through the use of a large set of Hubble Space Telescope (HST) observations. The latter include existing WFPC 2 images in the V and I bands, obtained at ~4.5‧ and 10' radial distances, as well as a series of deep images in the J and H bands obtained w…

2000 The Astrophysical Journal
eHST 48
On the possibility of ground-based direct imaging detection of extra-solar planets: the case of TWA-7
DOI: 10.48550/arXiv.astro-ph/9912500 Bibcode: 2000A&A...354L...9N

Neuhäuser, R.; Huélamo, N.; Brandner, W. +5 more

We show that ground-based direct imaging detection of extra-solar planets is possible with current technology. As an example, we present evidence for a possible planetary companion to the young T Tauri star 1RXSJ104230.3-334014 (=TWA-7), discovered by ROSAT as a member of the nearby TW Hya association. In an HST NICMOS F160W image, an object is de…

2000 Astronomy and Astrophysics
eHST 48
A Distance-Independent Age for the Globular Cluster M92
DOI: 10.1086/301560 Bibcode: 2000AJ....120.1884G

Grundahl, F.; Stetson, P. B.; Andersen, M. I. +2 more

We use deep Strömgren CCD photometry to determine the age of the globular cluster M92 (NGC 6341) from the [(v-y)0,c0]-diagram. Besides being completely independent of distance, this color-color plot has the further advantage that it is not very sensitive to the amount of foreground interstellar absorption. The main disadvanta…

2000 The Astronomical Journal
Hipparcos 48