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The Optical/Near-Infrared Counterpart of the INTEGRAL Obscured Source IGR J16318-4848: An sgB[e] in a High-Mass X-Ray Binary?
DOI: 10.1086/424869 Bibcode: 2004ApJ...616..469F

Filliatre, P.; Chaty, S.

The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003 January 29. The high-energy spectrum exhibits such a high column density that the source is undetectable in X-rays below 2 keV. On 2003 February 23-25, we triggered our Target of Opportunity (ToO) program using the EMMI and SOFI instruments on the New Technology T…

2004 The Astrophysical Journal
INTEGRAL 113
GRAPES, Grism Spectroscopy of the Hubble Ultra Deep Field: Description and Data Reduction
DOI: 10.1086/422582 Bibcode: 2004ApJS..154..501P

Cimatti, A.; Daddi, E.; Panagia, N. +19 more

We present deep unbiased spectroscopy of the Hubble Ultra Deep Field (UDF) carried out using the slitless grism spectroscopy mode of the Advanced Camera for Surveys on the Hubble Space Telescope (HST). The Grism ACS Program for Extragalactic Science (GRAPES) achieves continuum detection as faint as zAB=27.2 using 40 orbits (9.2×104…

2004 The Astrophysical Journal Supplement Series
eHST 111
Ultra-High-Precision Velocity Measurements of Oscillations in α Centauri A
DOI: 10.1086/381434 Bibcode: 2004ApJ...600L..75B

Butler, R. Paul; Bedding, Timothy R.; Marcy, Geoffrey W. +5 more

We have made differential radial velocity measurements of the star α Centauri A using two spectrographs, the UV-Visual Echelle Spectrograph (UVES) and the University College London Echelle Spectrograph (UCLES), both with iodine absorption cells for wavelength referencing. Stellar oscillations are clearly visible in the time series. After removing …

2004 The Astrophysical Journal
SOHO 111
Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton
DOI: 10.1051/0004-6361:20031471 Bibcode: 2004A&A...416..713G

Audard, M.; Güdel, M.; Linsky, J. L. +2 more

We report results from a comprehensive study of the nearby M dwarf Proxima Centauri with the XMM-Newton satellite, using simultaneously its X-ray detectors and the Optical Monitor with its U band filter. We find strongly variable coronal X-ray emission, with flares ranging over a factor of 100 in peak flux. The low-level emission is found to be co…

2004 Astronomy and Astrophysics
XMM-Newton 111
Cluster observations of continuous reconnection at the magnetopause under steady interplanetary magnetic field conditions
DOI: 10.5194/angeo-22-2355-2004 Bibcode: 2004AnGeo..22.2355P

Balogh, A.; Klecker, B.; Rème, H. +9 more

Available from http://www.copernicus.org/site/EGU/annales/22/7/2355.htm?FrameEngine=false;

2004 Annales Geophysicae
Cluster 110
Observing the Formation of the Hubble Sequence in the Great Observatories Origins Deep Survey
DOI: 10.1086/378556 Bibcode: 2004ApJ...600L.139C

Grogin, Norman A.; Lucas, Ray A.; Ravindranath, Swara +6 more

Understanding the physical formation of the Hubble sequence remains one of the most important unsolved astrophysical problems. Searches for protodisks and proto-elliptical galaxies can now be effectively done using deep wide-field Hubble Space Telescope images taken with the new Advanced Camera for Surveys. Through an analysis of the concentration…

2004 The Astrophysical Journal
eHST 110
The Fluctuating Intergalactic Radiation Field at Redshifts z = 2.3-2.9 from He II and H I Absorption toward HE 2347-4342
DOI: 10.1086/379924 Bibcode: 2004ApJ...600..570S

Shull, J. Michael; Kriss, Gerard A.; Tumlinson, Jason +2 more

We provide an in-depth analysis of the He II and H I absorption in the intergalactic medium (IGM) at redshifts z=2.3-2.9 toward HE 2347-4342, using spectra from the Far Ultraviolet Spectroscopic Explorer and the Ultraviolet-Visual Echelle Spectrograph on the Very Large Telescope. Following up on our earlier study, we focus here on two major topics…

2004 The Astrophysical Journal
eHST 110
Indications of a Large Fraction of Spectroscopic Binaries among Nuclei of Planetary Nebulae
DOI: 10.1086/382156 Bibcode: 2004ApJ...602L..93D

Bond, Howard E.; De Marco, Orsola; Harmer, Dianne +1 more

Previous work indicates that about 10% of planetary-nebula nuclei (PNNi) are photometrically variable short-period binaries with periods of hours to a few days. These systems have most likely descended from common-envelope (CE) interactions in initially much wider binaries. Population-synthesis studies suggest that these very close pairs could be …

2004 The Astrophysical Journal
IUE 110
Study of the properties and spectral energy distributions of the Herbig AeBe stars HD 34282 and HD 141569
DOI: 10.1051/0004-6361:20034561 Bibcode: 2004A&A...419..301M

Rauer, H.; Schneider, J.; Eiroa, C. +21 more

We present a study of the stellar parameters, distances and spectral energy distributions (SEDs) of HD 34282 and HD 141569, two pre-main sequence Herbig AeBe stars. Both objects have been reported to show ``anomalous positions'' in the HR diagram in the sense that they appear below the main sequence. A signifi…

2004 Astronomy and Astrophysics
Hipparcos IUE 110
Flux and energy modulation of redshifted iron emission in NGC 3516: implications for the black hole mass
DOI: 10.1111/j.1365-2966.2004.08392.x Bibcode: 2004MNRAS.355.1073I

Iwasawa, K.; Fabian, A. C.; Miniutti, G.

We report on the tentative detection of the modulation of a transient, redshifted Fe Kα emission feature in the X-ray spectrum of the Seyfert galaxy NGC 3516. The detection of the spectral feature at 6.1 keV, in addition to a stable 6.4-keV line, has been reported previously. We find, on reanalysing the XMM-Newton data, that the feature varies sys…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 109