Search Publications

X-Ray Properties of an Unbiased Hard X-Ray-detected Sample of Active Galactic Nuclei
DOI: 10.1086/525274 Bibcode: 2008ApJ...674..686W

Mushotzky, Richard F.; Tueller, Jack; Markwardt, Craig +1 more

The Swift gamma-ray observatory's Burst Alert Telescope (BAT) has detected a sample of AGNs based solely on their hard X-ray flux (14-195 keV). In this paper we present for the first time XMM-Newton X-ray spectra for 22 BAT AGNs with no previously analyzed X-ray spectra. If our sources are a representative sample of the BAT AGNs, as we claim, our …

2008 The Astrophysical Journal
XMM-Newton 92
Deep Advanced Camera for Surveys Imaging in the Globular Cluster NGC 6397: the Cluster Color-Magnitude Diagram and Luminosity Function
DOI: 10.1088/0004-6256/135/6/2141 Bibcode: 2008AJ....135.2141R

Anderson, Jay; Dotter, Aaron; Rich, R. Michael +9 more

We present the color-magnitude diagram (CMD) from deep Hubble Space Telescope imaging in the globular cluster NGC 6397. The Advanced Camera for Surveys (ACS) was used for 126 orbits to image a single field in two colors (F814W, F606W) 5' SE of the cluster center. The field observed overlaps that of archival WFPC2 data from 1994 and 1997 which were…

2008 The Astronomical Journal
eHST 91
3C 454.3 Reveals the Structure and Physics of Its "Blazar Zone"
DOI: 10.1086/526419 Bibcode: 2008ApJ...675...71S

Madejski, Greg M.; Sikora, Marek; Moderski, RafaŁ

Recent multiwavelength observations of 3C 454.3, in particular during its giant outburst in 2005, put severe constraints on the location of the "blazar zone," its dissipative nature, and high-energy radiation mechanisms. As the optical, X-ray, and millimeter light curves indicate, a significant fraction of the jet energy must be released in the vi…

2008 The Astrophysical Journal
INTEGRAL 91
Characteristic size and shape of the mirror mode structures in the solar wind at 0.72 AU
DOI: 10.1029/2008GL033793 Bibcode: 2008GeoRL..3510106Z

Russell, C. T.; Zhang, T. L.; Glassmeier, K. -H. +10 more

We investigate the structure of mirror modes in the solar wind at 0.72 AU using Venus Express magnetic field measurements. The mirror mode structure is identified as the presence of magnetic depression or magnetic ``holes'' in the solar wind with little or no directional change across them. We determine the characteristic size and shape of these s…

2008 Geophysical Research Letters
VenusExpress 91
Tropical mountain glaciers on Mars: Altitude-dependence of ice accumulation, accumulation conditions, formation times, glacier dynamics, and implications for planetary spin-axis/orbital history
DOI: 10.1016/j.icarus.2008.08.008 Bibcode: 2008Icar..198..305F

Head, James W.; Forget, Francois; Fastook, James L. +1 more

Fan-shaped deposits up to ∼166,000 km in area are found on the northwest flanks of the huge Tharsis Montes volcanoes in the tropics of Mars. Recent spacecraft data have confirmed earlier hypotheses that these lobate deposits are glacial in origin. Increased knowledge of polar-latitude terrestrial glacial analogs in the Antarctic Dry Valleys has be…

2008 Icarus
MEx 91
A comparison of coronal mass ejections identified by manual and automatic methods
DOI: 10.5194/angeo-26-3103-2008 Bibcode: 2008AnGeo..26.3103Y

Gopalswamy, N.; Michalek, G.; Yashiro, S.

Coronal mass ejections (CMEs) are related to many phenomena (e.g. flares, solar energetic particles, geomagnetic storms), thus compiling of event catalogs is important for a global understanding these phenomena. CMEs have been identified manually for a long time, but in the SOHO era, automatic identification methods are being developed. In order t…

2008 Annales Geophysicae
SOHO 91
The shape of the dark matter halo in the early-type galaxy NGC 2974
DOI: 10.1111/j.1365-2966.2007.12680.x Bibcode: 2008MNRAS.383.1343W

Krajnović, Davor; van de Ven, Glenn; Morganti, Raffaella +3 more

We present HI observations of the elliptical galaxy NGC 2974, obtained with the Very Large Array. These observations reveal that the previously detected HI disc in this galaxy is in fact a ring. By studying the harmonic expansion of the velocity field along the ring, we constrain the elongation of the halo and find that the underlying gravitationa…

2008 Monthly Notices of the Royal Astronomical Society
eHST 90
First Imaging of Coronal Mass Ejections in the Heliosphere Viewed from Outside the Sun Earth Line
DOI: 10.1007/s11207-007-9083-6 Bibcode: 2008SoPh..247..171H

Howard, Russell A.; Bewsher, Danielle; Davis, Christopher J. +13 more

We show for the first time images of solar coronal mass ejections (CMEs) viewed using the Heliospheric Imager (HI) instrument aboard the NASA STEREO spacecraft. The HI instruments are wide-angle imaging systems designed to detect CMEs in the heliosphere, in particular, for the first time, observing the propagation of such events along the Sun - Ea…

2008 Solar Physics
SOHO 90
Systematic Infrared 2.5-5 µm Spectroscopy of Nearby Ultraluminous Infrared Galaxies with AKARI
DOI: 10.1093/pasj/60.sp2.S489 Bibcode: 2008PASJ...60S.489I

Nakagawa, Takao; Shirahata, Mai; Imanishi, Masatoshi +4 more

We report on the results of systematic infrared 2.5-5 µm spectroscopy of 45 nearby ultraluminous infrared galaxies (ULIRGs) at z < 0.3 using AKARI IRC. This paper investigates whether the luminosities of these ULIRGs are dominated by starburst activity, or alternatively, whether optically elusive buried active galactic nuclei (AGNs) are e…

2008 Publications of the Astronomical Society of Japan
AKARI 90
Disks around CQ Tauri and MWC 758: dense PDR or gas dispersal?
DOI: 10.1051/0004-6361:200809523 Bibcode: 2008A&A...488..565C

Chapillon, E.; Guilloteau, S.; Dutrey, A. +1 more

Context: The overall properties of disks surrounding intermediate PMS stars (HAe) are not yet well constrained by current observations. The disk inclination, which significantly affects spectral energy distribution modeling, is often unknown.
Aims: We attempted to resolve the disks around CQ Tau and MWC 758 to provide accurate constraints on t…

2008 Astronomy and Astrophysics
IUE 90