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HST observations of the protoplanetary nebula OH 231.8+4.2: The structure of the jets and shocks
DOI: 10.1051/0004-6361:20020455 Bibcode: 2002A&A...389..271B

Sahai, R.; Sánchez Contreras, C.; Alcolea, J. +1 more

We present high-resolution images obtained with the WFPC2, on board the HST, of the protoplanetary nebula (PPN) OH 231.8+4.2. Hα and NII line emission and scattered light in the continuum at 6750 and 7910 Å were observed. We also discuss NIR NICMOS images from the HST archive. The images show with high accuracy the shape and excitation state of th…

2002 Astronomy and Astrophysics
eHST 56
ISO ammonia line absorption reveals a layer of hot gas veiling Sgr B2
DOI: 10.1051/0004-6361:20011765 Bibcode: 2002A&A...383..603C

Prusti, T.; Ceccarelli, C.; Caux, E. +7 more

We report the first results of the unbiased spectral high resolution survey obtained towards Sgr B2 with the Long Wavelength Spectrometer on board ISO. The survey detected more than one hundreds lines from several molecules. Ammonia is the molecule with the largest number (21) of detected lines in the survey. We detected NH3 transitions…

2002 Astronomy and Astrophysics
ISO 55
What Are the Hot R Coronae Borealis Stars?
DOI: 10.1086/340569 Bibcode: 2002AJ....123.3387D

De Marco, Orsola; Clayton, Geoffrey C.; Clark, J. S. +3 more

We investigate the evolutionary status of four stars: V348 Sgr, DY Cen, and MV Sgr in the Galaxy and HV 2671 in the LMC. These stars have in common random deep declines in visual brightness, which are characteristic of R Coronae Borealis (RCB) stars. RCB stars are typically cool hydrogen-deficient supergiants. The four stars studied in this paper …

2002 The Astronomical Journal
IUE 55
High-resolution observations and mass modelling of the CLASS gravitational lens B1152+199
DOI: 10.1046/j.1365-8711.2002.05043.x Bibcode: 2002MNRAS.330..205R

Biggs, A. D.; Browne, I. W. A.; Wilkinson, P. N. +5 more

We present a series of high-resolution radio and optical observations of the CLASS gravitational lens system B1152+199 obtained with the Multi-Element Radio-Linked Interferometer Network, Very Long Baseline Array and Hubble Space Telescope . Based on the milliarcsecond-scale substructure of the lensed radio components and precise optical astrometr…

2002 Monthly Notices of the Royal Astronomical Society
eHST 55
The Galaxy Octopole Moment as a Probe of Weak-Lensing Shear Fields
DOI: 10.1086/324202 Bibcode: 2002ApJ...564...65G

Natarajan, Priyamvada; Goldberg, David M.

In this paper, we introduce the octopole moment of the light distribution in galaxies as a probe of the weak-lensing shear field. While traditional ellipticity estimates of the local shear derived from the quadrupole moment are limited by the width of the intrinsic ellipticity distribution of background galaxies, the dispersion in the intrinsic oc…

2002 The Astrophysical Journal
eHST 55
On electron acceleration at CIR related shock waves
DOI: 10.1051/0004-6361:20020866 Bibcode: 2002A&A...391..749M

Mann, G.; Keppler, E.; Roelof, E. C. +1 more

The interaction of fast and slow speed solar wind streams leads to the formation of so-called corotating interaction regions (CIRs) in the heliosphere. These CIRs are often associated with shock waves, at which electrons are accelerated as observed by the Ulysses spacecraft. A correlation between the ratio of energetic electron fluxes at the cross…

2002 Astronomy and Astrophysics
Ulysses 55
Nuclear Stellar Disks in Spiral Galaxies
DOI: 10.1086/340486 Bibcode: 2002ApJ...573..131P

Scarlata, C.; Stiavelli, M.; Morelli, L. +4 more

We report evidence for nuclear stellar disks in three early-type spirals, namely, NGC 1425, NGC 3898, and NGC 4698, revealed by Wide Field Planetary Camera 2 F606W images out of a sample of 38 spiral galaxies, selected from the Hubble Space Telescope data archive. Adopting the photometric method introduced by Scorza & Bender, we derived their …

2002 The Astrophysical Journal
eHST 55
The status of Galactic field λ Bootis stars in the post-Hipparcos era
DOI: 10.1046/j.1365-8711.2002.05865.x Bibcode: 2002MNRAS.336.1030P

Kamp, I.; Paunzen, E.; Iliev, I. Kh. +1 more

The λ Bootis stars are Population I, late B- to early F-type stars, with moderate to extreme (up to a factor 100) surface underabundances of most Fe-peak elements and solar abundances of lighter elements (C, N, O and S). To put constraints on the various existing theories that try to explain these peculiar stars, we investigate the observational p…

2002 Monthly Notices of the Royal Astronomical Society
Hipparcos 55
On the origin of radial magnetic fields in the heliosphere
DOI: 10.1029/2002JA009434 Bibcode: 2002JGRA..107.1327G

Gosling, J. T.; Skoug, R. M.

Numerous examples of events wherein the heliospheric magnetic field (HMF) measured at a fixed point in space remains nearly radial for many hours have been reported in the literature. Such events are observed both in the normal solar wind and within disturbances driven by coronal mass ejections (CMEs). A very large fraction of these extended, near…

2002 Journal of Geophysical Research (Space Physics)
Ulysses 55
Timing analysis of the isolated neutron star RX J0720.4-3125
DOI: 10.1046/j.1365-8711.2002.05480.x Bibcode: 2002MNRAS.334..345Z

Cropper, Mark; Zavlin, Vyacheslav E.; Haberl, Frank +4 more

We present a combined analysis of XMM-Newton, Chandra and ROSAT observations of the isolated neutron star RX J0720.4-3125, spanning a total period of ~7yr. We develop a maximum likelihood periodogram for our analysis based on the ΔC statistic and the maximum likelihood method, which are appropriate for the treatment of sparse event lists. Our resu…

2002 Monthly Notices of the Royal Astronomical Society
XMM-Newton 55