Search Publications

Modulation of Jovian and galactic electrons in the heliosphere: 2. Radial transport of a few MeV electrons
DOI: 10.1029/2001JA000170 Bibcode: 2001JGR...10629313F

Fichtner, H.; Ferreira, S. E. S.; Potgieter, M. S. +3 more

Previously, the latitudinal transport of ~7 MeV electrons was studied by comparing the results of a newly developed three-dimensional model, based on the numerical solution of Parker's transport equation including the Jovian source, with Ulysses observations. Here, the radial transport of ~16 MeV electrons is studied by comparing the model results…

2001 Journal of Geophysical Research
Ulysses 56
Interstellar Bubbles in Two Young H II Regions
DOI: 10.1086/322067 Bibcode: 2001AJ....122..921N

Danforth, Charles W.; Nazé, Yaël; Chu, You-Hua +3 more

Massive stars are expected to produce wind-blown bubbles in the interstellar medium; however, ring nebulae, suggesting the existence of bubbles, are rarely seen around main-sequence O stars. To search for wind-blown bubbles around main-sequence O stars, we have obtained high-resolution Hubble Space Telescope WFPC2 images and high-dispersion echell…

2001 The Astronomical Journal
eHST 56
A new model of solar EUV irradiance variability: 1. Model formulation
DOI: 10.1029/2000JA000282 Bibcode: 2001JGR...10615745W

Mariska, J. T.; Warren, H. P.; Lean, J.

We present a new model of solar irradiance variability at extreme ultraviolet wavelengths (EUV, 50-1200 Å). In this model, quiet Sun, coronal hole, and active region intensities for optically thin emission lines are computed from emission measure distributions determined from spectrally and spatially resolved observations. For optically thick emis…

2001 Journal of Geophysical Research
SOHO 56
Are There Blue, Massive E/S0 Galaxies at z<1? Kinematics of Blue Spheroidal Galaxy Candidates
DOI: 10.1086/322081 Bibcode: 2001AJ....122..750I

Gebhardt, Karl; Faber, S. M.; Willmer, Christopher N. A. +5 more

Several recent studies find that 10%-50% of morphologically selected field early-type galaxies at redshifts z<~1 have blue colors indicative of recent star formation. Such ``blue spheroids'' might be massive early-type galaxies with active star formation, perhaps induced by recent merger events. Alternatively, they could be starbursting, low-ma…

2001 The Astronomical Journal
eHST 56
Cluster magnetic field observations in the magnetosheath: four-point measurements of mirror structures
DOI: 10.5194/angeo-19-1421-2001 Bibcode: 2001AnGeo..19.1421L

Balogh, A.; Horbury, T. S.; Lucek, E. A. +7 more

The Cluster spacecraft have returned the first simultaneous four-point measurements of the magnetosheath. We present an analysis of data recorded on 10 November 2000, when the four spacecrafts observed an interval of strong mirrorlike activity. Correlation analysis between spacecraft pairs is used to examine the scale size of the mirror structures…

2001 Annales Geophysicae
Cluster 56
Observation of Polar Plumes at High Solar Altitudes
DOI: 10.1086/318221 Bibcode: 2001ApJ...546..569D

Plunkett, S. P.; Andrews, M. D.; DeForest, C. E.

Using the Large-Angle Spectrometric Coronagraph (LASCO) aboard the Solar and Heliospheric Observatory (SOHO) spacecraft, we have imaged polar plumes extending 30 Rsolar from disk center in the image plane and ~45 Rsolar in three-dimensional space, a factor of 2-3 farther than previous imaging measurements and well into the co…

2001 The Astrophysical Journal
SOHO 56
Seeing Galaxies through Thick and Thin. III. Hubble Space Telescope Imaging of the Dust in Backlit Spiral Galaxies
DOI: 10.1086/319386 Bibcode: 2001AJ....121.1442K

White, Raymond E., III; Keel, William C.

We present analysis of Wide Field Planetary Camera 2 imaging of two spiral galaxies partially backlit by elliptical or S0 systems in the pairs AM 1316-241 and AM 0500-620, as well as the (probably spiral) foreground system in NGC 1275. Images in B and I are used to determine the reddening curve of dust in these systems. The foreground spiral compo…

2001 The Astronomical Journal
eHST 56
Optical spectroscopy and photometry of the neutron star RX J1856.5-3754
DOI: 10.1051/0004-6361:20011272 Bibcode: 2001A&A...378..986V

Kulkarni, S. R.; van Kerkwijk, M. H.

We present spectroscopy and imaging with the Very Large Telescope (VLT) of the neutron star RX J1856.5-3754. Little is known about the nature of this source other than that it is a nearby hot neutron star. Our VLT spectrum does not show any strong emission or absorption features. With considerable care to photometric calibration…

2001 Astronomy and Astrophysics
eHST 56
Late AGB Magnetic Cycles: Magnetohydrodynamic Solutions for the Hubble Space Telescope Planetary Nebula Rings
DOI: 10.1086/323072 Bibcode: 2001ApJ...560..928G

García-Segura, Guillermo; López, José Alberto; Franco, José

The Hubble Space Telescope (HST) has revealed the existence of multiple, regularly spaced, and faint concentric shells around some planetary nebulae. Here we present two- (and a half) dimensional magnetohydrodynamic numerical simulations of the effects of a solar-like magnetic cycle, with periodic polarity inversions, in the slow wind of an asympt…

2001 The Astrophysical Journal
eHST 56
High-resolution spectroscopy of the low-mass X-ray binary EXO 0748-67
DOI: 10.1051/0004-6361:20000053 Bibcode: 2001A&A...365L.277C

Kahn, S. M.; Brinkman, A. C.; den Herder, J. W. +2 more

We present initial results from observations of the low-mass X-ray binary EXO 0748-67 with the Reflection Grating Spectrometer on board the XMM-Newton Observatory. The spectra exhibit discrete structure due to absorption and emission from ionized neon, oxygen, and nitrogen. We use the quantitative constraints imposed by the spec…

2001 Astronomy and Astrophysics
XMM-Newton 55