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Distinguishing Local and Global Influences on Galaxy Morphology: A Hubble Space Telescope Comparison of High and Low X-Ray Luminosity Clusters
DOI: 10.1086/338056 Bibcode: 2002ApJ...566..123B

Kneib, J. -P.; Smith, G. P.; Smail, Ian +6 more

We present a morphological analysis of 17 X-ray-selected clusters at z~0.25, imaged uniformly with the Hubble Space Telescope Wide Field Planetary Camera 2 (WFPC2). Eight of these clusters comprise a subsample selected for their low X-ray luminosities (<~1044 ergs s-1), called the low-LX sample. The remaining ni…

2002 The Astrophysical Journal
eHST 45
On the Temperature Structure of M87
DOI: 10.1086/343757 Bibcode: 2002ApJ...580..815M

Molendi, Silvano

We revisit the XMM-Newton observation of M87, focusing our attention on the temperature structure. We find that spectra for most regions of M87 can be adequately fitted by single-temperature models. Only in a few regions, which are cospatial with the east and southwest radio arms, do we find evidence of a second temperature. The cooler component (…

2002 The Astrophysical Journal
XMM-Newton 44
The Timing of Flares Associated with the Two Dynamical Types of Solar Coronal Mass Ejections
DOI: 10.1086/342275 Bibcode: 2002ApJ...574L..97Z

Golub, L.; Zhang, M.; Burkepile, J. +1 more

In this Letter, we consider a sample of Transition Region and Coronal Explorer flare-associated solar coronal mass ejections (CMEs) and study the timing behavior of the flares associated with fast or slow CMEs. We find that flares associated with fast CMEs tend to happen within half an hour of the CME onsets, while the timing of flares associated …

2002 The Astrophysical Journal
SOHO 44
The Broadband Afterglow of GRB 980329
DOI: 10.1086/342175 Bibcode: 2002ApJ...577..155Y

Price, P. A.; Harrison, F. A.; Galama, T. J. +15 more

We present radio observations of the afterglow of the bright γ-ray burst GRB 980329 made between 1 month and several years after the burst, a reanalysis of previously published submillimeter data, and late-time optical and near-infrared (NIR) observations of the host galaxy. From the absence of a spectral break in the optical/NIR colors of the hos…

2002 The Astrophysical Journal
eHST 43
Solar and Heliospheric Observatory Ultraviolet Coronagraph Spectrometer and Yohkoh Soft X-Ray Telescope Observations of the High-Temperature Corona above an Active Region Complex
DOI: 10.1086/342616 Bibcode: 2002ApJ...578..979K

Fineschi, Silvano; Raymond, John C.; Li, Jing +4 more

We present the results of Solar and Heliospheric Observatory Ultraviolet Coronagraph Spectrometer (SOHO/UVCS) and Yohkoh Soft X-Ray Telescope (SXT) observations above an active region complex (AR 8194, 8195, and 8198) at the southeast limb on 1998 April 6-7. This active region complex appears to be the base of a small streamer seen by the Large An…

2002 The Astrophysical Journal
SOHO 43
XMM-Newton Detection of Hard X-Ray Emission in the Nitrogen-Type Wolf-Rayet Star WR 110
DOI: 10.1086/340307 Bibcode: 2002ApJ...572..477S

Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel +1 more

We have used the excellent sensitivity of XMM-Newton to obtain the first high-quality X-ray spectrum of a Wolf-Rayet (W-R) star that is not known to be a member of a binary system. Our target, the nitrogen-type star WR 110 (HD 165688), was also observed and detected with the Very Large Array at four different frequencies. The radio flux density in…

2002 The Astrophysical Journal
XMM-Newton 43
The X-Ray Source at the Center of the Cassiopeia A Supernova Remnant
DOI: 10.1086/339277 Bibcode: 2002ApJ...569..275M

Tiengo, A.; Mereghetti, S.; Israel, G. L.

We present the first results of an XMM-Newton observation of the central X-ray source in the Cas A supernova remnant. The spectrum can be fitted equally well with an absorbed steep power law (αph~3, NH~1.5×1022 cm-2) or with a bremsstrahlung with temperature kT~2.4 keV and NH~1022 c…

2002 The Astrophysical Journal
XMM-Newton 43
Hubble Space Telescope/NICMOS Observations of Terzan 5: Stellar Content and Structure of the Core
DOI: 10.1086/339874 Bibcode: 2002ApJ...571..818C

Cohn, Haldan N.; Lugger, Phyllis M.; Edmonds, Peter D. +1 more

We report results from Hubble Space Telescope/NICMOS imaging of the extremely dense core of the globular cluster Terzan 5. This highly obscured bulge cluster contains a low-mass X-ray binary and at least two millisecond pulsars, with evidence for a large millisecond pulsar population. It has been estimated to have one of the highest collision rate…

2002 The Astrophysical Journal
eHST 43
X-Ray Bright Points and Photospheric Bipoles during Cycles 22 and 23
DOI: 10.1086/324306 Bibcode: 2002ApJ...564.1042S

Pevtsov, Alexei A.; Sattarov, Isroil; Hojaev, Alisher S. +1 more

We use the Yohkoh soft X-ray telescope (SXT) full-disk images made from 1993 to 2000 to manually identify X-ray bright points (XBPs). We also employ the National Solar Observatory (Kitt Peak) full-disk longitudinal magnetograms made between 1992 April and 2001 April and an automatic procedure to identify photospheric bipoles whose magnetic field s…

2002 The Astrophysical Journal
SOHO 43
Thermal Pressures in Neutral Clouds inside the Local Bubble, as Determined from C I Fine-Structure Excitations
DOI: 10.1086/343796 Bibcode: 2002ApJ...580..938J

Jenkins, Edward B.

High-resolution spectra covering the absorption features from interstellar C I were recorded for four early-type stars with spectrographs on the Hubble Space Telescope, in a program to measure the fine-structure excitation of this atom within neutral clouds inside or near the edge of the Local Bubble, a volume of hot (T~106K) gas that e…

2002 The Astrophysical Journal
eHST 42