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The optical counterpart of the ultraluminous X-ray source NGC 5204 X-1
DOI: 10.1046/j.1365-8711.2002.05852.x Bibcode: 2002MNRAS.335L..67G

Knigge, C.; Roberts, T. P.; Lira, P. +1 more

We use archival HST/WFPC2 V- and I-band images to show that the optical counterpart to the ultraluminous X-ray source NGC 5204 X-1, reported by Roberts et al., is composed of two sources separated by 0.5 arcsec. We have also identified a third source as a possible counterpart, which lies 0.8 arcsec from the nominal X-ray position. Point spread fun…

2002 Monthly Notices of the Royal Astronomical Society
eHST 50
The dual dust chemistries of planetary nebulae with [WCL] central stars
DOI: 10.1046/j.1365-8711.2002.05350.x Bibcode: 2002MNRAS.332..879C

Barlow, M. J.; Liu, X. -W.; Cohen, Martin +1 more

The rather rare class of central stars of planetary nebulae that show very low-excitation Wolf-Rayet spectra has been a subject of great interest, particularly in the infrared, since its discovery in the late 1960s. Further peculiarities have been found with the advent of infrared spectroscopy from ISO. Notably, these objects simultaneously betray…

2002 Monthly Notices of the Royal Astronomical Society
ISO 50
Infrared Fe II Emission in Narrow-Line Seyfert 1 Galaxies
DOI: 10.1086/324598 Bibcode: 2002ApJ...565..140R

Pastoriza, M. G.; Prato, L.; Rodríguez-Ardila, A. +1 more

We obtained 0.8-2.4 µm spectra at a resolution of 320 km s-1 of four narrow-line Seyfert 1 galaxies in order to study the near-infrared properties of these objects. We focus on the analysis of the Fe II emission in that region and the kinematics of the low-ionization broad lines. We show that the 1 µm Fe II lines (λ9997, λ10…

2002 The Astrophysical Journal
eHST 50
Multi-wavelength observations of an X-class flare without a coronal mass ejection.
DOI: 10.1023/A:1014211528863 Bibcode: 2002SoPh..205..325G

van Driel-Gesztelyi, L.; Culhane, J. L.; Green, L. M. +2 more

Developments in our knowledge of coronal mass ejections (CMEs) have shown that many of these transients occur in association with solar flares. On the occasions when there is a common occurrence of the eruption and the flare, it is most likely that the flare is of high intensity and/or long-duration (Burkepile, Hundhausen, and Webb, 1994; Munro et…

2002 Solar Physics
SOHO 50
A Far Ultraviolet Spectroscopic Explorer Survey of Interstellar O VI Absorption in the Small Magellanic Cloud
DOI: 10.1086/339323 Bibcode: 2002ApJ...569..233H

Hoopes, Charles G.; Sembach, Kenneth R.; Savage, Blair D. +2 more

We present the results of a Far Ultraviolet Spectroscopic Explorer (FUSE) survey of O VI λ1031.93 and λ1037.62 absorption toward 18 OB stars in the Small Magellanic Cloud (SMC). The FUSE data are of very high quality, allowing a detailed study of the coronal temperature gas in the SMC. We find that O VI is ubiquitous in the SMC, with a detection a…

2002 The Astrophysical Journal
eHST 50
Diffuse X-ray emission from the planetary nebula NGC 7009
DOI: 10.1051/0004-6361:20020330 Bibcode: 2002A&A...387L...1G

Gruendl, R. A.; Chu, Y. -H.; Guerrero, M. A.

XMM-Newton EPIC observations of the planetary nebula (PN) NGC 7009, the Saturn Nebula, have detected extended X-ray emission in its central cavity. The diffuse X-ray emission must originate in the shocked fast stellar wind. The spectra show that the temperature of the hot gas is 1.8x 106 K. The rms density derived from the volume emissi…

2002 Astronomy and Astrophysics
XMM-Newton 49
Optical Slitless Spectroscopy of Large Magellanic Cloud Planetary Nebulae: A Study of the Emission Lines and Morphology
DOI: 10.1086/341146 Bibcode: 2002ApJ...575..178S

Mutchler, Max; Blades, J. Chris; Balick, Bruce +3 more

Hubble Space Telescope Space Telescope Imaging Spectrograph slitless spectroscopy of LMC planetary nebulae (PNs) is the ideal tool to study their morphology and their ionization structures at once. We present the results from a group of 29 PNs that have been spatially resolved, for the first time, in all the major optical lines. Images in the ligh…

2002 The Astrophysical Journal
eHST 49
A new, cleaner colour-magnitude diagram for the metal-rich globular cluster NGC 6528. Velocity dispersion in the Bulge, age and proper motion of NGC 6528
DOI: 10.1051/0004-6361:20011771 Bibcode: 2002A&A...385...67F

Feltzing, S.; Johnson, R. A.

Using two epochs of HST/WFPC2 images of the metal-rich globular cluster NGC 6528 we derive the proper motions of the stars and use them to separate the stars belonging to NGC 6528 from those of the Galactic bulge. The stellar sequences in the resulting colour-magnitude diagram for the cluster are significantly better determined than in previously …

2002 Astronomy and Astrophysics
eHST 49
The Luminosity Functions of Old and Intermediate-Age Globular Clusters in NGC 3610
DOI: 10.1086/340808 Bibcode: 2002AJ....124..147W

Kundu, Arunav; Whitmore, Bradley C.; Schweizer, François +1 more

The Wide Field Planetary Camera 2 on board the Hubble Space Telescope (HST) has been used to obtain high-resolution images of NGC 3610, a dynamically young elliptical galaxy in a group environment. These observations supersede shorter, undithered HST observations in which an intermediate-age population of globular clusters was discovered. The new …

2002 The Astronomical Journal
eHST 49
Discovery and Implications of a New Large-Scale Stellar Bar in NGC 5248
DOI: 10.1086/340974 Bibcode: 2002ApJ...570L..55J

Laine, Seppo; Jogee, Shardha; Knapen, Johan H. +3 more

For decades, the grand-design SAB spiral galaxy NGC 5248 has been postulated to host a short bar of semimajor axis 22" (1.6 kpc). From dynamical and morphological arguments, however, we argue that its spiral structure is being driven by a large-scale bar whose corotation radius lies at ~115" (8.6 kpc). Our estimate is based partially on a deep R-b…

2002 The Astrophysical Journal
eHST 49