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The Star Formation Rate Intensity Distribution Function: Implications for the Cosmic Star Formation Rate History of the Universe
DOI: 10.1086/339774 Bibcode: 2002ApJ...570..492L

Chen, Hsiao-Wen; Lanzetta, Kenneth M.; Pascarelle, Sebastian +2 more

We address the effects of cosmological surface brightness dimming on observations of faint galaxies by examining the distribution of ``unobscured'' star formation rate intensities versus redshift. We use the star formation rate intensity distribution function to assess the ultraviolet luminosity density versus redshift, based on our photometry and…

2002 The Astrophysical Journal
eHST 125
ISO spectroscopy of compact H II regions in the Galaxy. II. Ionization and elemental abundances
DOI: 10.1051/0004-6361:20011504 Bibcode: 2002A&A...381..606M

Kessler, M. F.; Morisset, C.; Schaerer, D. +9 more

Based on the ISO spectral catalogue of compact H II regions by \cite{peeters:catalogue}, we present a first analysis of the hydrogen recombination and atomic fine-structure lines originated in the ionized gas. The sample consists of 34 H II regions located at galactocentric distances between RGal,= 0 and 15 kpc. The SWS H I recombinatio…

2002 Astronomy and Astrophysics
ISO 125
Sources of the solar wind at solar activity maximum
DOI: 10.1029/2001JA000306 Bibcode: 2002JGRA..107.1488N

Smith, E. J.; Neugebauer, M.; Zurbuchen, T. H. +2 more

The photospheric sources of solar wind observed by the Ulysses and ACE spacecraft from 1998 to early 2001 are determined through a two-step mapping process. Solar wind speed measured at the spacecraft is used in a ballistic model to determine a foot point on a source surface at a solar distance of 2.5 solar radii. A potential-field source-surface …

2002 Journal of Geophysical Research (Space Physics)
Ulysses 125
WIYN Open Cluster Study. X. The K-Band Magnitude of the Red Clump as a Distance Indicator
DOI: 10.1086/339027 Bibcode: 2002AJ....123.1603G

Sarajedini, Ata; Grocholski, Aaron J.

In an effort to improve the utility of the helium-burning red clump luminosity as a distance indicator, we explore the sensitivity of the K-band red clump absolute magnitude [MK(RC)] to metallicity and age. We rely upon JK photometry for 14 open clusters and two globular clusters from the Second Incremental Data Release of the Two Micro…

2002 The Astronomical Journal
Hipparcos 124
Crystalline silicate dust around evolved stars. I. The sample stars
DOI: 10.1051/0004-6361:20011550 Bibcode: 2002A&A...382..184M

Waters, L. B. F. M.; Barlow, M. J.; Tielens, A. G. G. M. +1 more

This is the first paper in a series of three where we present the first comprehensive inventory of solid state emission bands observed in a sample of 17 oxygen-rich circumstellar dust shells surrounding evolved stars. The data were taken with the Short and Long Wavelength Spectrographs on board of the Infrared Space Observatory (ISO) and cover the…

2002 Astronomy and Astrophysics
ISO 124
Ten Low-Mass Companions from the Keck Precision Velocity Survey
DOI: 10.1086/338768 Bibcode: 2002ApJ...568..352V

Butler, R. Paul; Vogt, Steven S.; Fischer, Debra A. +4 more

Ten new companions have emerged from the Keck precision Doppler velocity survey, with minimum (Msini) masses ranging from 0.8 MJUP to 0.34 Msolar. Five of these are planet candidates with Msini<12 MJUP, two are brown dwarf candidates with Msini~30 MJUP, and three are low-mass stellar companions. Hippa…

2002 The Astrophysical Journal
Hipparcos 124
Magnetic Topology of Impulsive and Gradual Solar Energetic Particle Events
DOI: 10.1086/341149 Bibcode: 2002ApJ...571L..63R

Reames, Donald V.

We examine the magnetic topology at the Sun that leads to the two classes of impulsive and gradual solar energetic particle (SEP) events so as to address new observations that seem to blur this classification, for example, that coronal mass ejections (CMEs) can accompany events of both classes. In our model, the unusual element abundances in impul…

2002 The Astrophysical Journal
SOHO 124
The Star Formation History of the Large Magellanic Cloud
DOI: 10.1086/337985 Bibcode: 2002ApJ...566..239S

Cole, Andrew A.; Gallagher, John S., III; Stetson, Peter B. +1 more

Using WFPC2 on board the Hubble Space Telescope, we have created deep color-magnitude diagrams in the V and I passbands for approximately 105 stars in a field at the center of the LMC bar and another in the disk. The main-sequence luminosity functions (LFs) from 19<=V<=23.5, the red clump and horizontal branch morphologies, and th…

2002 The Astrophysical Journal
eHST 124
Intracluster Red Giant Stars in the Virgo Cluster
DOI: 10.1086/339735 Bibcode: 2002ApJ...570..119D

Ciardullo, Robin; Sigurdsson, Steinn; Durrell, Patrick R. +2 more

We have used the Wide Field Planetary Camera 2 on the Hubble Space Telescope to obtain deep F814W images of a blank field in the Virgo Cluster located 41' northwest of M87. We perform star counts in that field and in another Virgo field observed by Ferguson, Tanvir, & von Hippel and show that when compared to the Hubble Deep Field-North and Hu…

2002 The Astrophysical Journal
eHST 124
Rhessi and Trace Observations of the 21 April 2002 x1.5 Flare
DOI: 10.1023/A:1022422019779 Bibcode: 2002SoPh..210..341G

Krucker, Säm; Gallagher, Peter T.; Dennis, Brian R. +2 more

Observations of the X1.5 flare on 21 April 2002 are reviewed using the Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) and the Transition Region and Coronal Explorer (TRACE). The major findings are as follows: (1) The 3-25 keV X-rays started < 4 min before the EUV (195 Å) emission suggesting that the initial energy release heated …

2002 Solar Physics
SOHO 124