Search Publications
The XMM-NEWTON Long Look of NGC 1365: Lack of a High/Soft State in its Ultraluminous X-Ray Sources
Bianchi, S.; Elvis, M.; Fabbiano, G. +3 more
Based on our long (~300 ks) 2007 XMM-Newton observation of the Seyfert galaxy NGC 1365, we report here on the spectral and timing behavior of two ultraluminous X-ray sources (ULXs), which had previously reached isotropic X-ray luminosities L X ≈ 4 × 1040 erg s-1 (0.3-10 keV band). In 2007, they were in a lower stat…
Stereoscopic Reconstruction from STEREO/EUV Imagers Data of the Three-dimensional Shape and Expansion of an Erupting Prominence
Bemporad, A.
On 2007 May 9, a prominence eruption was observed in the He II λ304 filter by the two EUV Imagers (EUVI) telescopes aboard the STEREO A and B spacecrafts. The high spatial resolution (~1farcs5 pixel-1) EUVI images have been used to infer via triangulation the three-dimensional (3D) shape and orientation of the prominence sime12 minutes …
Deep Keck u-Band Imaging of the Hubble Ultra Deep Field: A Catalog of z ~ 3 Lyman Break Galaxies
Rafelski, Marc; Chen, Hsiao-Wen; Wolfe, Arthur M. +3 more
We present a sample of 407 z ~ 3 Lyman break galaxies (LBGs) to a limiting isophotal u-band magnitude of 27.6 mag in the Hubble Ultra Deep Field. The LBGs are selected using a combination of photometric redshifts and the u-band drop-out technique enabled by the introduction of an extremely deep u-band image obtained with the Keck I telescope and t…
Discovery of X-Ray Emission from the Wolf-Rayet Star WR 142 of Oxygen Subtype
Hamann, W. -R.; Chu, Y. -H.; Oskinova, L. M. +2 more
We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR 142 with the XMM-Newton X-ray telescope. Being of spectral subtype WO2, WR 142 is a massive star in a very advanced evolutionary stage shortly before its explosion as a supernova or γ-ray burst. This is the first detection of X-ray emission from a WO-type star…
Estimating the Chromospheric Absorption of Transition Region Moss Emission
De Pontieu, Bart; McIntosh, Scott W.; Hansteen, Viggo H. +1 more
Many models for coronal loops have difficulty explaining the observed EUV brightness of the transition region, which is often significantly less than theoretical models predict. This discrepancy has been addressed by a variety of approaches including filling factors and time-dependent heating, with varying degrees of success. Here, we focus on an …
Optical and X-ray Observations of M31N 2007-12b: An Extragalactic Recurrent Nova with a Detected Progenitor?
Shafter, A. W.; Page, K. L.; Bode, M. F. +4 more
We report combined optical and X-ray observations of nova M31N 2007-12b. Optical spectroscopy obtained 5 days after the 2007 December outburst shows evidence of very high ejection velocities (FWHM Hα sime 4500 km s-1). In addition, Swift X-ray data show that M31N 2007-12b is associated with a Super-Soft Source (SSS) which appeared betwe…
Energetic Particle Observations and Propagation in the Three-dimensional Heliosphere During the 2006 December Events
Lario, D.; Forsyth, R. J.; Cohen, C. M. S. +9 more
We report observations of solar energetic particles obtained by the HI-SCALE and COSPIN/LET instruments onboard Ulysses during the period of isolated but intense solar activity in 2006 December, in the declining phase of the solar activity cycle. We present measurements of particle intensities and also discuss observations of particle anisotropies…
The Motion of Water Masers in the Pre-Planetary Nebula IRAS 16342-3814
Sahai, R.; Morris, M. R.; Claussen, M. J.
We present high angular resolution observations, using the Very Long Baseline Array of the NRAO4The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc., of the high-velocity water masers toward the "water fountain" pre-planetary nebul…
Coronal Implosion and Particle Acceleration in the Wake of a Filament Eruption
Wang, Haimin; Liu, Rui
We study the evolution of a group of TRACE 195 Å coronal loops overlying a reverse S-shaped filament on 2001 June 15. These loops were initially pushed upward with the filament ascending and kinking slowly, but as soon as the filament rose explosively, they began to contract at a speed of ~100 km s-1, and sustained for at least 12 minut…
A Smoking Gun in the Carina Nebula
Hamaguchi, Kenji; Corcoran, Michael F.; Petre, Rob +8 more
The Carina Nebula is one of the youngest, most active sites of massive star formation in our Galaxy. In this nebula, we have discovered a bright X-ray source that has persisted for ~30 years. The soft X-ray spectrum, consistent with kT ~ 128 eV blackbody radiation with mild extinction, and no counterpart in the near- and mid-infrared wavelengths i…