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XMM-Newton and the Pleiades - I. Bright coronal sources and the X-ray emission from intermediate-type stars
DOI: 10.1046/j.1365-8711.2003.06991.x Bibcode: 2003MNRAS.345..714B

Briggs, K. R.; Pye, J. P.

We present results of X-ray spectral and timing analyses of solar-like (spectral types F5-K8) and intermediate-type (B4-F4) Pleiads observed in a 40-ks XMM-Newton EPIC exposure, probing X-ray luminosities (LX) up to a factor 10 fainter than previous studies using the ROSAT PSPC. All eight solar-like members have `quasi-steady'LX

2003 Monthly Notices of the Royal Astronomical Society
XMM-Newton 55
Infrared spectroscopy of faint 15 mu m sources in the Hubble Deep Field South: First hints at the properties of the sources of the IR background
DOI: 10.1051/0004-6361:20030351 Bibcode: 2003A&A...403..501F

Berta, S.; Aussel, H.; Elbaz, D. +8 more

We present a spectroscopic analysis of a sample of 21 galaxies with z = 0.2-1.5 drawn from a 25 square arcmin ultra-deep ISOCAM survey at lambdaeff =15 mu m centered in the WFPC-2 Hubble Deep Field South. Near-infrared spectra are reported for 18 ISO sources, carried out with ISAAC on the VLT, aimed at detecting the redshifted Halp…

2003 Astronomy and Astrophysics
ISO eHST 55
Hubble Space Telescope imaging and ground-based spectroscopy of old nova shells - II. The bipolar shell of the slow nova HR Del
DOI: 10.1046/j.1365-8711.2003.06906.x Bibcode: 2003MNRAS.344.1219H

O'Brien, T. J.; Harman, D. J.

We present Hubble Space Telescope (HST) WFPC2 imaging of HR Del in filters centred on the lines of Hα, [N II] and [O III], with corresponding William Herschel Telescope (WHT) ISIS slit spectroscopy for the lines of Hα, Hβ, [N II] and [O III]. The data show that the ejected shell of HR Del is composed of many small bright knots. These are distribut…

2003 Monthly Notices of the Royal Astronomical Society
eHST 55
On the structure and kinematics of nebulae around LBVs and LBV candidates in the LMC
DOI: 10.1051/0004-6361:20030921 Bibcode: 2003A&A...408..205W

Weis, K.

We present a detailed analysis of the morphology and kinematics of nebulae around LBVs and LBV candidates in the Large Magellanic Cloud. HST images and high-resolution Echelle Spectra were used to determine the size, shape, brightness, and expansion velocities of the LBV nebulae around R 127, R 143, and S 61. For S Dor, R 71, R 99, and R 84 we dis…

2003 Astronomy and Astrophysics
eHST 55
Chandra Observation of the Edge-on Galaxy NGC 3556 (M108): Violent Galactic Disk-Halo Interaction Revealed
DOI: 10.1086/379010 Bibcode: 2003ApJ...598..969W

Wang, Q. Daniel; Irwin, Judith A.; Chaves, Tara

We present a 60 ks Chandra ACIS-S observation of the isolated edge-on spiral galaxy NGC 3556, together with a multiwavelength analysis of various discrete X-ray sources and diffuse X-ray features. Among 33 discrete X-ray sources detected within the IB=25 mag arcsec-2 isophote ellipse of the galaxy, we identify a candidate for…

2003 The Astrophysical Journal
eHST 55
X-Ray Evidence of a Buried Active Galactic Nucleus in UGC 5101
DOI: 10.1086/379503 Bibcode: 2003ApJ...596L.167I

Nakagawa, Takao; Imanishi, Masatoshi; Terashima, Yuichi +1 more

We present X-ray observations of the ultraluminous infrared galaxy, UGC 5101, thought to contain a buried active galactic nucleus (AGN) based on observations in other wave bands. We detected an absorbed hard component at greater than 3 keV, as well as soft emission in the energy range 0.5-2 keV. The soft X-ray component, possibly due to a modestly…

2003 The Astrophysical Journal
XMM-Newton 55
The Canada-UK Deep Submillimeter Survey. VII. Optical and Near-Infrared Identifications for the 14 Hour Field
DOI: 10.1086/381217 Bibcode: 2003ApJ...597..680W

Clements, D. L.; Dunne, L.; Eales, S. +5 more

We present the multiwavelength identifications for 23 sources in the Canada-UK Deep Submillimeter Survey (CUDSS) 14h field. The identifications have been selected on the basis of radio and near-infrared data, and we argue that, to our observational limits, both are effective at selecting the correct counterparts of the SCUBA sources. We…

2003 The Astrophysical Journal
ISO eHST 55
X-Ray Spectroscopy of the Low-Mass X-Ray Binaries 2S 0918-549 and 4U 1543-624: Evidence for Neon-rich Degenerate Donors
DOI: 10.1086/379188 Bibcode: 2003ApJ...599..498J

Chakrabarty, Deepto; Juett, Adrienne M.

We present high-resolution spectroscopy of the neutron star/low-mass X-ray binaries 2S 0918-549 and 4U 1543-624 with the High Energy Transmission Grating Spectrometer on board the Chandra X-Ray Observatory and the Reflection Grating Spectrometer on board XMM-Newton. Previous low-resolution spectra of both sources showed a broad, linelike feature a…

2003 The Astrophysical Journal
XMM-Newton 55
Observations of the SW Sextantis Star DW Ursae Majoris with the Far Ultraviolet Spectroscopic Explorer
DOI: 10.1086/378605 Bibcode: 2003AJ....126.2473H

Szkody, Paula; Hoard, D. W.; Long, Knox S. +2 more

We present an analysis of the first far-ultraviolet observations of the SW Sextantis type cataclysmic variable DW Ursae Majoris, obtained in 2001 November with the Far Ultraviolet Spectroscopic Explorer. The time-averaged spectrum of DW UMa shows a rich assortment of emission lines (plus some contamination from interstellar absorption lines includ…

2003 The Astronomical Journal
IUE 55
Simultaneous Ultraviolet and X-Ray Spectroscopy of the Seyfert 1 Galaxy NGC 5548. I. Physical Conditions in the Ultraviolet Absorbers
DOI: 10.1086/376792 Bibcode: 2003ApJ...594..116C

Kaastra, J. S.; Turner, T. J.; Kraemer, S. B. +9 more

We present new UV spectra of the nucleus of the Seyfert 1 galaxy NGC 5548, which we obtained with the Space Telescope Imaging Spectrograph at high spectral resolution, in conjunction with simultaneous Chandra X-Ray Observatory spectra. Taking advantage of the low UV continuum and broad emission-line fluxes, we have determined that the deepest UV a…

2003 The Astrophysical Journal
IUE eHST 55