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Chandra, EUVE, HST, and VLA Multiwavelength Campaign on HR 1099: Instrumental Capabilities, Data Reduction, and Initial Results
DOI: 10.1086/319051 Bibcode: 2001ApJ...549..554A

Ayres, Thomas R.; Brown, Alexander; Drake, Jeremy J. +4 more

In mid-September of 1999, a multiwavelength campaign was carried out on the coronally active RS Canum Venaticorum binary HR 1099 (K1 IV+G5 V P=2.84 days), during commissioning of the High Energy Transmission Grating Spectrometer (HETGS) of the Chandra X-ray Observatory (CXO). The coordinated program involved the Extreme Ultraviolet Explorer (EUVE)…

2001 The Astrophysical Journal
eHST 77
Dust in the Tycho, Kepler and Crab supernova remnants
DOI: 10.1051/0004-6361:20010447 Bibcode: 2001A&A...373..281D

Dwek, E.; Lagage, P. O.; Cesarsky, C. J. +1 more

SuperNova Remnants (SNR) have been extensively studied in radio, X-rays and optical, but barely in the InfraRed (IR). From IRAS observations, SNR are known to be IR emitters, but the origin of the emission is difficult to assess because of the limited angular and spectral resolution of IRAS observations. ISO follow-up observations of the Cassiopei…

2001 Astronomy and Astrophysics
ISO 76
Space Telescope Imaging Spectrograph Echelle Observations of the Seyfert Galaxy NGC 4151: Physical Conditions in the Ultraviolet Absorbers
DOI: 10.1086/320244 Bibcode: 2001ApJ...551..671K

Gull, T. R.; Kraemer, S. B.; Crenshaw, D. M. +7 more

We have examined the physical conditions in intrinsic UV-absorbing gas in the Seyfert galaxy NGC 4151, using echelle spectra obtained with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope on 1999 July 19. We confirm the presence of the kinematic components detected in earlier Goddard High Resolution Spectrograph (GHRS)…

2001 The Astrophysical Journal
eHST 76
Speckle Interferometry of New and Problem Hipparcos Binaries. II. Observations Obtained in 1998-1999 from McDonald Observatory
DOI: 10.1086/321096 Bibcode: 2001AJ....121.3224M

Mason, Brian D.; Hartkopf, William I.; Holdenried, Ellis R. +1 more

The Hipparcos satellite made measurements of over 9734 known double stars, 3406 new double stars, and 11,687 unresolved but possible double stars. The high angular resolution afforded by speckle interferometry makes it an efficient means to confirm these systems from the ground, which were first discovered from space. Because of its coverage of a …

2001 The Astronomical Journal
Hipparcos 76
Homogenization of the Stellar Population along Late-Type Spiral Galaxies
DOI: 10.1086/322126 Bibcode: 2001AJ....122.1298G

dos Anjos, S.; Gadotti, D. A.

We present a study of the broadband UBV color profiles for 257 Sbc barred and nonbarred galaxies, using photoelectric aperture photometry data from the literature. Using robust statistical methods, we have estimated the color gradients of the galaxies, as well as the total and bulge mean colors. A comparative photometric study using CCD images was…

2001 The Astronomical Journal
eHST 76
The central region of M 31 observed with XMM-Newton. II. Variability of the individual sources
DOI: 10.1051/0004-6361:20011228 Bibcode: 2001A&A...378..800O

Pietsch, W.; Read, A. M.; Tiengo, A. +13 more

We present the results of a study of the variability of X-ray sources in the central 30 arcmin of the nearby Andromeda Galaxy (M 31) based on XMM-Newton Performance Verification observations. Two observations of this field, with a total exposure time of about 50 ks, were performed in June and December of 2000. We found 116 sources brighter than a …

2001 Astronomy and Astrophysics
XMM-Newton 76
The central region of M 31 observed with XMM-Newton. I. Group properties and diffuse emission
DOI: 10.1051/0004-6361:20000243 Bibcode: 2001A&A...365L.195S

Pietsch, W.; Read, A. M.; Tiengo, A. +13 more

We present the results of a study based on an XMM-Newton Performance Verification observation of the central 30' of the nearby spiral galaxy M 31. In the 34-ks European Photon Imaging Camera (EPIC) exposure, we detect 116 sources down to a limiting luminosity of 6 x 1035 erg s-1 (0.3-12 keV, d=760 kpc). The luminosity distrib…

2001 Astronomy and Astrophysics
XMM-Newton 76
The Southern Crab from a New Perspective
DOI: 10.1086/320665 Bibcode: 2001ApJ...553..211C

Livio, Mario; Corradi, Romano L. M.; Munari, Ulisse +2 more

New Hubble Space Telescope images and Cerro Tololo Inter-American Observatory echelle spectra of the nebula around the symbiotic Mira Henize 2-104 are presented. The nebula consists of two nested hourglass-shaped structures and a collimated polar jet. Spatiokinematical modeling shows that all three outflows were ejected during approximately the sa…

2001 The Astrophysical Journal
eHST 76
Coronal Mass Ejection of 2000 July 14 Flare Event: Imaging from Near-Sun to Earth Environment
DOI: 10.1086/322332 Bibcode: 2001ApJ...559.1180M

Pick, M.; Kaiser, M. L.; Ipavich, F. M. +6 more

We report the results of our investigation of interplanetary effects caused by the large solar flare (X5.7/3B) that occurred on 2000 July 14. In association with this event a bright, fast, halo coronal mass ejection (CME) was observed. The analysis of multiwavelength, high-cadence images obtained from the Nançay Radioheliograph shows the on-disk s…

2001 The Astrophysical Journal
SOHO 75
Temporal Variations of the Solar Rotation Rate at High Latitudes
DOI: 10.1086/323701 Bibcode: 2001ApJ...559L..67A

Basu, Sarbani; Antia, H. M.

Frequency splitting coefficients from Global Oscillation Network Group and Michelson Doppler Imager observations covering the period 1995-2001 are used to study temporal variations in the solar rotation rate at high latitudes. The torsional oscillation pattern in the Sun is known to penetrate to a depth of about 0.1 Rsolar with alternat…

2001 The Astrophysical Journal
SOHO 75