Search Publications

Using a Hipparcos-derived Hertzsprung-Russell Diagram to Limit the Metallicity Scatter of Stars in the Hyades: Are Stars Polluted?
DOI: 10.1086/340809 Bibcode: 2002AJ....124..400Q

Quillen, A. C.

Hipparcos parallaxes and proper motions have made it possible to construct Hertzsprung-Russell (H-R) diagrams of nearby clusters with unprecedented accuracy. The standard deviation of high-fidelity, nonbinary, nonvariable stars about a model stellar evolution isochrone in the Hyades cluster is about 0.04 mag. We use this deviation to estimate an u…

2002 The Astronomical Journal
Hipparcos 28
Ulysses Cosmic Ray and Solar Particle Investigation/Kiel Electron Telescope observations: Charge sign dependence and spatial gradients during the 1990-2000 A > 0 solar magnetic cycle
DOI: 10.1029/2001JA000329 Bibcode: 2002JGRA..107.1274H

Kunow, H.; Wibberenz, G.; Ferreira, S. E. S. +10 more

Ulysses, launched in October 1990, began its second out-of-ecliptic orbit in September 1997. From 1991 to mid-2000, solar polar magnetic field observations indicate a magnetic field pointing outward over the northern polar region (A > 0 epoch). While the first fast latitude scan in 1994/1995 was performed around solar minimum, the second Ulysse…

2002 Journal of Geophysical Research (Space Physics)
Ulysses 28
Multi wavelength investigation of the eruption of a sigmoidal quiescent filament
DOI: 10.1051/0004-6361:20020309 Bibcode: 2002A&A...387..317M

Delaboudinière, J. P.; Marqué, Ch.; Lantos, P.

We report the first observation of a filament eruption in the metric and decimetric range, where the behavior of the filament can be followed during the event via thermal radio emission diagnostics. The event, occurring on February 28th 2001, involved a quiescent filament in a sigmoid magnetic configuration, whose eruption is triggered by the birt…

2002 Astronomy and Astrophysics
SOHO 27
Young Stellar Nuclei in Lenticular Galaxies: NGC 5574 and NGC 7457
DOI: 10.1086/342243 Bibcode: 2002ApJ...577..668S

Chavushyan, V. H.; Sil'chenko, O. K.; Afanasiev, V. L. +1 more

The stellar population properties in the centers of NGC 5574 and NGC 7457 (two lenticular galaxies previously shown to have radially homogeneous blue optical-band colors) are studied by means of integral-field spectroscopy. The compact nuclei of the galaxies appear to be chemically distinct: in NGC 5574 the nucleus is distinguished by a higher tha…

2002 The Astrophysical Journal
eHST 27
The Differential Emission Measure Distribution in the Multiloop Corona
DOI: 10.1086/345469 Bibcode: 2002ApJ...580L..79A

Aschwanden, Markus J.

This is a rebuttal of a recent Letter on the inadequacy of temperature measurements in the solar corona through narrowband filter and line ratios by Martens et al. We simulate the differential emission measure (DEM) distribution of a multiloop corona and find that the temperature profile of individual loops can be retrieved with narrowband filter …

2002 The Astrophysical Journal
SOHO 27
SDSS J124602.54 + 011318.8: A Highly Luminous Optical Transient at z = 0.385
DOI: 10.1086/341887 Bibcode: 2002ApJ...576..673V

Schneider, Donald P.; York, Donald G.; Hurley, Kevin +30 more

We report the discovery of a highly luminous optical transient (OT), SDSS J124602.54 + 011318.8, associated with a galaxy at a redshift of 0.385. In this paper, we consider the possibility that the OT may be a gamma-ray burst (GRB) afterglow. Three sets of images and two sets of spectra were obtained as part of the normal operations of the Sloan D…

2002 The Astrophysical Journal
Ulysses 27
µJy radio sources in the cluster MS1054-03
DOI: 10.1046/j.1365-8711.2002.05023.x Bibcode: 2002MNRAS.330...17B

Franx, M.; van Dokkum, P. G.; Röttgering, H. J. A. +1 more

An extremely deep 5-GHz radio observation is presented of the rich cluster MS1054-03 at redshift 34 radio sources are detected down to a 6σ level of 32µJy, compared with about 25 expected from previous blank-field radio source count determinations; the sources giving rise to these excess counts lie predominantly within 2arcmin (~700kpc) of t…

2002 Monthly Notices of the Royal Astronomical Society
eHST 27
Extreme X-ray variability in the luminous quasar PDS 456
DOI: 10.1046/j.1365-8711.2002.06038.x Bibcode: 2002MNRAS.336L..56R

O'Brien, P. T.; Reeves, J. N.; Pounds, K. A. +1 more

We present evidence from BeppoSAX and XMM-Newton of extreme X-ray variability in the high-luminosity radio-quiet quasar PDS 456, the most luminous known active galactic nucleus (AGN) at z < 0.3. Repeated X-ray flaring is found in PDS 456, over the duration of the 340-ks long BeppoSAX observation. The X-ray flux doubles in just 30 ks, whilst the…

2002 Monthly Notices of the Royal Astronomical Society
XMM-Newton 27
The Redshift of a Lensing Galaxy in PMN J0134-0931
DOI: 10.1086/342784 Bibcode: 2002ApJ...575L..51H

Bowen, David V.; Hall, Patrick B.; Brinkmann, J. +5 more

The Sloan Digital Sky Survey (SDSS) automatically targeted as a quasar candidate the recently discovered, gravitationally lensed, extremely reddened z=2.2 quasar PMN 0134-0931. The SDSS spectrum exhibits Ca II absorption at z=0.76451, which we identify as the redshift of a lensing galaxy. Hubble Space Telescope imaging shows that components C, D, …

2002 The Astrophysical Journal
eHST 27
Real-time forecasting of ICME shock arrivals at L1 during the "April Fool’s Day" epoch: 28 March  21 April 2001
DOI: 10.5194/angeo-20-937-2002 Bibcode: 2002AnGeo..20..937S

Dryer, M.; Smith, Z.; Fry, C. D. +5 more

The Sun was extremely active during the "April Fool’s Day" epoch of 2001. We chose this period between a solar flare on 28 March 2001 to a final shock arrival at Earth on 21 April 2001. The activity consisted of two presumed helmet-streamer blowouts, seven M-class flares, and nine X-class flares, the last of which was behind the west limb. We have…

2002 Annales Geophysicae
SOHO 27