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High resolution X-ray spectroscopy of zeta Puppis with the XMM-Newton reflection grating spectrometer
DOI: 10.1051/0004-6361:20000093 Bibcode: 2001A&A...365L.312K

Mewe, R.; Güdel, M.; Leutenegger, M. A. +5 more

We present the first high resolution X-ray spectrum of the bright O4Ief supergiant star zeta Puppis, obtained with the Reflection Grating Spectrometer on-board XMM-Newton. The spectrum exhibits bright emission lines of hydrogen-like and helium-like ions of nitrogen, oxygen, neon, magnesium, and silicon, as well as neon-like ions of iron. The lines…

2001 Astronomy and Astrophysics
IUE XMM-Newton 182
Central Structural Parameters of Early-Type Galaxies as Viewed with Nicmos on the Hubble Space Telescope
DOI: 10.1086/321175 Bibcode: 2001AJ....122..653R

Ravindranath, Swara; Filippenko, Alexei V.; Ho, Luis C. +2 more

We present surface photometry for the central regions of a sample of 33 early-type (E, S0, and S0/a) galaxies observed at 1.6 µm (H band) using the Hubble Space Telescope. Dust absorption has less of an impact on the galaxy morphologies in the near-infrared than found in previous work based on observations at optical wavelengths. When presen…

2001 The Astronomical Journal
eHST 181
The Formation of a Prominence in Active Region NOAA 8668. I. SOHO/MDI Observations of Magnetic Field Evolution
DOI: 10.1086/322491 Bibcode: 2001ApJ...560..476C

Qiu, Jiong; Wang, Haimin; Chae, Jongchul +3 more

We have studied the evolution of the photospheric magnetic field in active region NOAA 8668 for 3 days while the formation of a reverse S-shaped filament proceeded. From a set of full-disk line-of-sight magnetograms taken by the Michelson Doppler Imager (MDI) on board the Solar and Heliospheric Observatory (SOHO), we have found a large canceling m…

2001 The Astrophysical Journal
SOHO 181
CHIANTI-An Atomic Database for Emission Lines. IV. Extension to X-Ray Wavelengths
DOI: 10.1086/320854 Bibcode: 2001ApJS..134..331D

Young, P. R.; Del Zanna, G.; Dere, K. P. +1 more

CHIANTI provides a database of atomic energy levels, wavelengths, radiative transition probabilities, and electron excitation data for a large number of ions of astrophysical interest. It also includes a suite of Interactive Data Language programs to calculate optically thin synthetic spectra and to perform spectral analysis and plasma diagnostics…

2001 The Astrophysical Journal Supplement Series
SOHO 180
Mayall II=G1 in M31: Giant Globular Cluster or Core of a Dwarf Elliptical Galaxy?
DOI: 10.1086/321166 Bibcode: 2001AJ....122..830M

Djorgovski, S. G.; Jablonka, P.; Sarajedini, A. +3 more

Mayall II=G1 is one of the brightest globular clusters belonging to M31, the Andromeda galaxy. Our observations with the Wide Field and Planetary Camera (WFPC2) on board the Hubble Space Telescope (HST) provide photometric data for the I versus V-I and V versus V-I color-magnitude diagrams. They reach stars with magnitudes fainter than V=27 mag, w…

2001 The Astronomical Journal
eHST 180
A Multiwavelength Study of the Young Star Clusters and Interstellar Medium in the Antennae Galaxies
DOI: 10.1086/322278 Bibcode: 2001ApJ...561..727Z

Whitmore, Bradley C.; Fall, S. Michael; Zhang, Qing

We report on a multiwavelength study of the relationship between young star clusters in the Antennae galaxies (NGC 4038/9) and their interstellar environment, with the goal of understanding the formation and feedback effects of star clusters in merging galaxies. This is possible for the first time because various new observations (from X-rays to r…

2001 The Astrophysical Journal
eHST 180
Near-Sun and near-Earth manifestations of solar eruptions
DOI: 10.1029/2000JA004025 Bibcode: 2001JGR...10625261G

Kaiser, M. L.; Gopalswamy, N.; Bougeret, J. -L. +1 more

We compare the near-Sun and near-Earth manifestations of solar eruptions that occurred during November 1994 to June 1998. We compared white-light coronal mass ejections, metric type II radio bursts, and extreme ultraviolet wave transients (near the Sun) with interplanetary (IP) signatures such as decameter-hectometric type II bursts, kilometric ty…

2001 Journal of Geophysical Research
SOHO 178
Complex resonance absorption structure in the X-ray spectrum of IRAS 13349+2438
DOI: 10.1051/0004-6361:20000081 Bibcode: 2001A&A...365L.168S

Kaastra, J. S.; Clavel, J.; Behar, E. +8 more

The luminous infrared-loud quasar IRAS 13349+2438 was observed with the XMM-Newton Observatory as part of the Performance Verification program. The spectrum obtained by the Reflection Grating Spectrometer (RGS) exhibits broad (v ~ 1400 km s-1 FWHM) absorption lines from highly ionized elements including hydrogen- and …

2001 Astronomy and Astrophysics
XMM-Newton 178
XMM-Newton observations of M 87 and its X-ray halo
DOI: 10.1051/0004-6361:20000092 Bibcode: 2001A&A...365L.181B

Böhringer, H.; Dos Santos, S.; Guainazzi, M. +10 more

We report performance verification observations of the giant elliptical galaxy M 87 in the Virgo Cluster with the MOS, pn, and optical monitor instruments on board of XMM-Newton. With the energy sensitive imaging instruments MOS and pn we obtain the first spatially constrained X-ray spectra of the nucleus and the jet of the galaxy. The good photon…

2001 Astronomy and Astrophysics
XMM-Newton 177
First light measurements with the XMM-Newton reflection grating spectrometers: Evidence for an inverse first ionisation potential effect and anomalous Ne abundance in the Coronae of HR 1099
DOI: 10.1051/0004-6361:20000047 Bibcode: 2001A&A...365L.324B

Kaastra, J. S.; Mewe, R.; Audard, M. +15 more

The RS CVn binary system HR 1099 was extensively observed by the XMM-Newton observatory in February 2000 as its first-light target. A total of 570 ks of exposure time was accumulated with the Reflection Grating Spectrometers (RGS). The integrated X-ray spectrum between 5-35 Å is of unprecedented quality and shows numerous features attributed to tr…

2001 Astronomy and Astrophysics
XMM-Newton 177