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The Gravitational Lens Candidate FBQ 1633+3134
DOI: 10.1086/318744 Bibcode: 2001AJ....121..611M

White, Richard L.; Gregg, Michael D.; Morgan, Nicholas D. +2 more

We present our ground-based optical imaging, spectral analysis, and high-resolution radio mapping of the gravitational lens candidate FBQ 1633+3134. This z=1.52, B=17.7 quasar appears double on CCD images with an image separation of 0.66" and a relatively constant flux ratio of ~3:1 across B, V, R, and I filters. A single 0.27 mJy radio source is …

2001 The Astronomical Journal
eHST 16
The Extreme-Ultraviolet Structure and Properties of a Newly Emerged Active Region
DOI: 10.1086/322447 Bibcode: 2001ApJ...558..411G

Gallagher, Peter T.; Phillips, Kenneth J. H.; Lee, Jeongwoo +2 more

The structure and properties of a newly emerged solar active region (NOAA Active Region 7985) are discussed using the Coronal Diagnostic Spectrometer (CDS) and the Extreme-Ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory. CDS obtained high-resolution EUV spectra in the 308-381 Å and 513-633 Å wavelength ranges, w…

2001 The Astrophysical Journal
SOHO 16
Low-angle scattering of protons on the XMM-Newton optics and effects on the on-board CCD detectors
DOI: 10.1109/23.983135 Bibcode: 2001ITNS...48.1815N

Evans, H.; Nieminen, P.; Daly, E. +3 more

Monte Carlo simulations are presented where protons are shown to propagate through X-ray telescope optics by grazing incidence scattering processes. If these protons reach charge coupled device (CCD) detectors in sufficient numbers, they can induce a radiation background, and at certain energies, the nonionising dose can cause degradation of the c…

2001 IEEE Transactions on Nuclear Science
XMM-Newton 16
Earthward directed CMEs seen in large-scale coronal magnetic field changes, SOHO LASCO coronagraph and solar wind
DOI: 10.1029/2001JA900041 Bibcode: 2001JGR...10625103L

Plunkett, S. P.; Mulligan, T.; Hoeksema, J. Todd +4 more

One picture of coronal mass ejection (CME) initiation relates these events to the expansion into space of previously closed coronal magnetic fields, often part of the helmet streamer belt. The work described here makes use of the potential field source surface model based on updated synoptic photospheric field maps to study the large-scale coronal…

2001 Journal of Geophysical Research
SOHO 16
Injection of energetic protons during solar eruption on 1999 May 9: Effect of flare and coronal mass ejection
DOI: 10.1051/0004-6361:20000148 Bibcode: 2001A&A...365..198T

Torsti, J.; Innes, D. E.; Kocharov, L. +2 more

A solar energetic particle (SEP) event was observed on 1999 May 9 by the Energetic and Relativistic Nuclei and Electron instrument (ERNE) onboard the Solar and Heliospheric Observatory (SOHO) spacecraft in association with a coronal mass ejection (CME) and X-ray flare at the western limb. Near flare onset the active region coronal loop structure w…

2001 Astronomy and Astrophysics
SOHO 15
Ultraviolet Broad Absorption Features and the Spectral Energy Distribution of the Quasar PG 1351+64
DOI: 10.1086/323437 Bibcode: 2001ApJ...562..152Z

Zheng, W.; Kriss, G. A.; Wang, J. X. +7 more

We present a moderate-resolution (~20 km s-1) spectrum of the mini-broad absorption line quasar (QSO) PG 1351+64 between 915 and 1180 Å, obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE). Additional low-resolution spectra at longer wavelengths were also obtained with the Hubble Space Telescope (HST) and ground-based telesc…

2001 The Astrophysical Journal
eHST 15
Fast Dust in the Heliosphere
DOI: 10.1023/A:1013888830386 Bibcode: 2001SSRv...99..151G

Grün, E.; Landgraf, M.

The dynamics of dust particles in the solar system is dominated by solar gravity, by solar radiation pressure, or by electromagnetic interaction of charged dust grains with the interplanetary magnetic field. For micron-sized or bigger dust particles solar gravity leads to speeds of about 30 to 40 km s^-1 at the Earth's distance. Smaller particles …

2001 Space Science Reviews
Ulysses 15
ISOCAM observations of the deep IRAS 60 micron sample in the NEP region. II. Comparison of ISO and IRAS galaxy counts
DOI: 10.1016/S1384-1076(01)00052-5 Bibcode: 2001NewA....6..265M

Aussel, H.; Franceschini, A.; De Zotti, G. +3 more

We have determined IRAS flux densities at positions of sources detected by our ISOCAM LW3 observations of the IRAS deep survey sample in the north ecliptic polar region [ApJS 63 (1987) 311]. Exploiting the higher angular resolution of ISOCAM to deal with confusion effects and properly correcting the fluxes for observational biases, we show that 60…

2001 New Astronomy
ISO 15
Absolute Magnitudes and Kinematic Parameters of the Subsystem of RR Lyrae Variables
DOI: 10.1134/1.1344262 Bibcode: 2001AstL...27..108D

Dambis, A. K.; Rastorguev, A. S.

The statistical parallax technique is applied to a sample of 262 RRab Lyrae variables with published photoelectric photometry, metallicities, and radial velocities and with measured absolute proper motions. Hipparcos, PPM, NPM, and the Four-Million Star Catalog (Volchkov et al. 1992) were used as the sources of proper motions; the proper motions f…

2001 Astronomy Letters
Hipparcos 15
Spectral imaging maps of AR Lacertae . I. Results from IUE observations in 1994 October
DOI: 10.1051/0004-6361:20000025 Bibcode: 2001A&A...365..128P

Pagano, I.; Linsky, J. L.; Rodonò, M. +4 more

In October 1994 the RS CVn eclipsing binary AR Lacertae was monitored by IUE during two orbital cycles. We have used 59 low resolution spectra, acquired in the range 1150-1950 Å, to derive light curves for emission lines formed at different temperatures between about 10 000 and 200 000 K and to study the flare signatures versus …

2001 Astronomy and Astrophysics
IUE 15