Search Publications

Connecting the Sun and the Solar Wind: Comparison of the Latitudinal Profiles of Coronal and Ulysses Measurements of the Fast Wind
DOI: 10.1086/319172 Bibcode: 2001ApJ...549L.253H

Habbal, Shadia Rifai; Woo, Richard

A quantitative comparison of the latitudinal profile of polarized brightness (pB) measurements nearest the Sun at 1.15 Rsolar by the Mauna Loa Solar Observatory K-Coronameter and Ulysses interplanetary measurements of the fast solar wind during its first south polar pass, at the declining phase of the solar cycle, is made for the first …

2001 The Astrophysical Journal
Ulysses 16
Hubble Space Telescope NICMOS Imaging of the Cores of M31 and M32
DOI: 10.1086/320407 Bibcode: 2001AJ....121.2549C

Rieke, Marcia J.; Corbin, Michael R.; O'Neil, Earl

We present 1.1, 1.6, and 2.2 µm images of the cores of the Local Group galaxies M31 and M32 obtained with the Near Infrared Camera and Multi-Object Spectrometer of the Hubble Space Telescope (HST). These images are also compared with optical images of the galaxies obtained with the HST Wide Field Planetary Camera 2 (WFPC2). In M31, the nucle…

2001 The Astronomical Journal
eHST 16
Periodic signals in Ulysses' energetic particle events upstream and downstream from the Jovian bow shock
DOI: 10.1016/S0032-0633(01)00018-6 Bibcode: 2001P&SS...49.1031M

Sarris, E. T.; Anagnostopoulos, G. C.; Marhavilas, P. K.

We present results from a statistical analysis of energetic particle events, observed by the Heliosphere instrument for spectra, composition, and anisotrophy at low energies (HI-SCALE) instrument onboard Ulysses, upstream from the bow shock of Jupiter, during the inbound and outbound trajectory of the spacecraft. A harmonic analysis on the intensi…

2001 Planetary and Space Science
Ulysses 16
Is SBS 0335-052 a young galaxy?
DOI: 10.1051/0004-6361:20010326 Bibcode: 2001A&A...371..429O

Östlin, G.; Kunth, D.

The metal-poor blue compact galaxy SBS 0335-052 has been put forward as a local primeval galaxy candidate, with a proposed age less than 108 years. If true, this would imply that galaxy formation was not confined to high red-shifts, but is still occurring in the local Universe, albeit at a slower rate. In this paper we show that some of…

2001 Astronomy and Astrophysics
eHST 16
An Ultraviolet Study of the Short-Period Binary OO Aquilae
DOI: 10.1086/318740 Bibcode: 2001AJ....121.1084H

Guinan, Edward F.; Hrivnak, Bruce J.; Ribas, Ignasi +1 more

OO Aql is a rare W UMa-type eclipsing binary in which the two solar-type stars may have only recently evolved into contact. The binary has an unusually high mass ratio (0.84) and a relatively long orbital period (0.506 days) for its spectral type (mid-G). Twelve ultraviolet spectra of OO Aql were obtained in 1988 with the International Ultraviolet…

2001 The Astronomical Journal
IUE 16
Speckle observations of binary systems measured by Hipparcos
DOI: 10.1051/0004-6361:20000550 Bibcode: 2001A&A...367..865P

Lampens, P.; Prieur, J. -L.; Aristidi, E. +4 more

From speckle observations made with the PISCO speckle camera at the Pic du Midi Observatory, we present high angular resolution astrometric data for 43 binary stars already observed by the Hipparcos satellite. This sample consists of mainly new Hipparcos eclipsing binaries with a visual companion closer than one arcsecond, chosen with the aim to s…

2001 Astronomy and Astrophysics
Hipparcos 16
Long-Slit Observations of Extended C II λ1335 Emission around V854 Centauri and RY Sagittarii
DOI: 10.1086/323065 Bibcode: 2001ApJ...560..986C

Clayton, G. C.; Ayres, T. R.

We have obtained long-slit far-ultraviolet (1150-1730 Å) spectra of the R Coronae Borealis (RCB) stars V854 Cen and RY Sgr near maximum light and pulsational phase zero with the Space Telescope Imaging Spectrograph on board the Hubble Space Telescope. The far-UV spectrum of each star shows a photospheric continuum rising steeply toward longer wave…

2001 The Astrophysical Journal
eHST 16
Mesogranulation and Turbulence in Photospheric Flows
DOI: 10.1023/A:1011813925550 Bibcode: 2001SoPh..202...27L

Lawrence, J. K.; Cadavid, A. C.; Ruzmaikin, A.

Below the scale of supergranules we find that cellular flows are present in the solar photosphere at two distinct size scales, approximately 2 Mm and 4 Mm, with distinct characteristic times. Simultaneously present in the flow is a non-cellular component, with turbulent scaling properties and containing 30% of the flow energy. These results are ob…

2001 Solar Physics
SOHO 16
The proper motions of fundamental stars. I. 1535 stars from the Basic FK5
DOI: 10.1051/0004-6361:20000010 Bibcode: 2001A&A...365..222G

Gontcharov, G. A.; Andronova, A. A.; Titov, O. A. +1 more

A direct combination of the positions given in the HIPPARCOS catalogue with astrometric ground-based catalogues having epochs later than 1939 allows us to obtain new proper motions for the 1535 stars of the Basic FK5. The results are presented as the catalogue Proper Motions of Fundamental Stars (PMFS), Part I. The median precision of the proper m…

2001 Astronomy and Astrophysics
Hipparcos 16
Nature of the boundary between open and closed magnetic field line regions at the Sun revealed by composition data and numerical models
DOI: 10.1029/2000JA000112 Bibcode: 2001JGR...10615869P

Riley, Pete; Gloeckler, George; Posner, Arik +5 more

Recently, Fisk et al. [1999] have presented a theory that describes a number of features of the large-scale coronal and heliospheric magnetic field. This theory predicts large-scale transport of magnetic flux across the boundaries of the polar coronal holes, which leads to reconnection processes of open field lines with preliminary closed magnetic…

2001 Journal of Geophysical Research
Ulysses 16