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Iron Abundance in the Intracluster Medium at High Redshift
Tozzi, P.; Mainieri, V.; Rosati, P. +3 more
We present the analysis of the X-ray spectra of 18 distant clusters of galaxies with redshift 0.3<z<1.3. Most of them were observed with the Chandra satellite in long exposures ranging from 36 to 180 ks. For two of the z>1 clusters, we also use deep XMM-Newton observations. Overall, these clusters probe the temperature range 3keV<~kT&l…
Multiwavelength observations revealing the evolution of the outburst of the black hole XTE J1118+480
Chaty, S.; Cui, W.; Shrader, C. R. +3 more
We report multiwavelength observations of the soft X-ray transient XTE J1118+480, which we observed with UKIRT, Hubble Space Telescope (HST), RXTE, Extreme Ultraviolet Explorer (EUVE) and many other instruments and facilities. Adding radio (Ryle Telescope, VLA), submillimetre (JCMT) and X-ray (Chandra and SAX) data from the literature, we assemble…
Hubble Space Telescope Paα and 1.9 Micron Imaging of Sagittarius A West
Scoville, N. Z.; Yusef-Zadeh, F.; Stolovy, S. R. +2 more
We present Hubble Space Telescope/NICMOS images at 0.2" resolution (Nyquist-sampled in the central 19") of the H I Paα emission line in a 70''(α)×90''(δ) region of the Galactic center centered on the nonthermal radio source Sgr A*. The majority of the emission arises from ionized gas in the minispiral in the central parsec. P…
Surface brightness profiles and structural parameters for globular clusters in the Fornax and Sagittarius dwarf spheroidal galaxies
Mackey, A. D.; Gilmore, G. F.
We present radial surface brightness profiles for all five globular clusters in the Fornax dwarf spheroidal galaxy, and for the four present members of the Sagittarius dwarf spheroidal galaxy. These profiles are derived from archival Hubble Space Telescope observations, and have been calculated using the same techniques with which we measured prof…
Formation scenarios for the young stellar associations between galactic longitudes l = 280degr - 360degr
Dias, W. S.; Lépine, J. R. D.; Sartori, M. J.
We investigate the spatial distribution, the space velocities and age distribution of the pre-main sequence (PMS) stars belonging to Ophiuchus, Lupus and Chamaeleon star-forming regions (SFRs), and of the young early-type star members of the Scorpius-Centaurus OB association. These young stellar associations extend over the galactic longitude rang…
Discovery of a magnetic field in the Slowly Pulsating B star zeta Cassiopeiae
Frémat, Y.; Neiner, C.; Wiersema, K. +5 more
The Nuclear Regions of the Seyfert Galaxy NGC 4151: Parsec-Scale H I Absorption and a Remarkable Radio Jet
Mundell, C. G.; Pedlar, A.; Wrobel, J. M. +1 more
Sensitive high angular and linear resolution radio images of the 240 pc radio jet in NGC 4151, imaged at linear resolutions of 0.3-2.6 pc using the VLBA and phased VLA at λ21 cm, are presented and reveal for the first time a faint, highly collimated jet (diameter <~1.4 pc) underlying discrete components, seen in lower resolution MERLIN and VLA …
A Survey for Circumstellar Disks around Young Substellar Objects
Tokunaga, Alan T.; Liu, Michael C.; Najita, Joan
We have completed the first systematic survey for disks around spectroscopically identified young brown dwarfs and very low mass stars. For a sample of 38 very cool objects in IC 348 and Taurus, we have obtained L'-band (3.8 µm) imaging with sufficient sensitivity to detect objects with and without disks. The sample should be free of selecti…
The INTEGRAL IBIS/ISGRI System Point Spread Function and Source Location Accuracy
Goldoni, P.; Rodriguez, J.; Foschini, L. +5 more
The imager on board INTEGRAL (IBIS) presently provides the most detailed sky images ever obtained at energies above 30 keV. The telescope is based on a coded aperture imaging system which allows to obtain sky images in a large field of view (29deg x 29deg) with an angular resolution of 12'. The System Point Spread Function of…
Chandra X-Ray Observations of the Spiral Galaxy M81
Wu, Kinwah; Tennant, Allyn F.; Swartz, Douglas A. +3 more
A Chandra X-Ray Observatory ACIS-S imaging observation is used to study the population of X-ray sources in the nearby Sab galaxy M81 (NGC 3031). A total of 177 sources are detected with 124 located within the D25 isophote to a limiting X-ray luminosity of ~3×1036 ergs s-1. Source positions, count rates, luminositie…