Search Publications

Obscured Active Galactic Nuclei and the X-Ray, Optical, and Far-Infrared Number Counts of Active Galactic Nuclei in the GOODS Fields
DOI: 10.1086/424891 Bibcode: 2004ApJ...616..123T

Brandt, William N.; Van Duyne, Jeffrey; Chary, Ranga-Ram +12 more

The deep X-ray, optical, and far-infrared fields that constitute the Great Observatories Origins Deep Survey (GOODS) are sensitive to obscured active galactic nuclei (AGNs; NH>~1022 cm-2) at the quasar epoch (z~2-3), as well as to unobscured AGNs as distant as z~7. Luminous X-ray emission is a sign of accretion …

2004 The Astrophysical Journal
eHST 163
The Origins of X-Ray Emission from the Hot Spots of FR II Radio Sources
DOI: 10.1086/422808 Bibcode: 2004ApJ...612..729H

Hardcastle, M. J.; Birkinshaw, M.; Worrall, D. M. +1 more

We use new and archival Chandra data to investigate the X-ray emission from a large sample of compact hot spots of FR II radio galaxies and quasars from the 3C catalog. We find that only the most luminous hot spots tend to be in good agreement with the predictions of a synchrotron self-Compton model with equipartition magnetic fields. At low hot s…

2004 The Astrophysical Journal
eHST 162
Magnetic Doppler imaging of 53 Camelopardalis in all four Stokes parameters
DOI: 10.1051/0004-6361:20031595 Bibcode: 2004A&A...414..613K

Petit, P.; Piskunov, N.; Wade, G. A. +5 more

We present the first investigation of the structure of the stellar surface magnetic field using line profiles in all four Stokes parameters. We extract the information about the magnetic field geometry and abundance distributions of the chemically peculiar star 53 Cam by modelling time-series of high-resolution spectropolarimetric observations wit…

2004 Astronomy and Astrophysics
SOHO 162
High-resolution imaging of the HeII λ4686 emission line nebula associated with the ultraluminous X-ray source in Holmberg II
DOI: 10.1111/j.1365-2966.2004.08020.x Bibcode: 2004MNRAS.351L..83K

Zezas, A.; Kaaret, P.; Ward, M. J.

We present Hubble Space Telescope images of the HeIII region surrounding the bright X-ray source in the dwarf irregular galaxy Holmberg II. Using Chandra, we find a position for the X-ray source of (J2000) with an uncertainty of 0.6 arcsec. We identify a bright, point-like optical counterpart centred in the nebula with the X-ray source. The optica…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 162
The Formation of Dust Lanes: Implications for Galaxy Evolution
DOI: 10.1086/386358 Bibcode: 2004ApJ...608..189D

Yoachim, Peter; Dalcanton, Julianne J.; Bernstein, Rebecca A.

From a survey of edge-on disks, we find that disk galaxies show a sharp, mass-dependent transition in the structure of their dusty ISM. In more massive, rapidly rotating disks with Vc>120kms-1, we see the well-defined dust lanes traditionally associated with edge-on galaxies. However, in more slowly rotating, lower mass ga…

2004 The Astrophysical Journal
eHST 161
The Role of Magnetic Reconnection in the Observable Features of Solar Eruptions
DOI: 10.1086/380900 Bibcode: 2004ApJ...602..422L

Raymond, J. C.; van Ballegooijen, A. A.; Lin, J.

There are two competing classes of models for coronal mass ejections (CMEs): those that assume a preexisting magnetic flux rope and those that can make a flux rope during the eruption by magnetic reconnection. The present work is based on the model with a preexisting flux rope. We investigate the evolution of morphological features of the magnetic…

2004 The Astrophysical Journal
SOHO 160
Downflow Motions Associated with Impulsive Nonthermal Emissions Observed in the 2002 July 23 Solar Flare
DOI: 10.1086/420768 Bibcode: 2004ApJ...605L..77A

Shibata, Kazunari; Shimojo, Masumi; Yokoyama, Takaaki +1 more

We present a detailed examination of downflow motions above flare loops observed in the 2002 July 23 flare. The extreme-ultraviolet images obtained with the Transition Region and Coronal Explorer show dark downflow motions (sunward motions) above the postflare loops, not only in the decay phase but also in the impulsive and main phases. We also fo…

2004 The Astrophysical Journal
SOHO 160
X-ray reflection in the narrow-line Seyfert 1 galaxy 1H 0707-495
DOI: 10.1111/j.1365-2966.2004.08036.x Bibcode: 2004MNRAS.353.1071F

Vaughan, S.; Fabian, A. C.; Boller, Th. +4 more

We apply a reflection-dominated model to the second XMM-Newton observation of the narrow-line Seyfert 1 galaxy 1H 0707-495. As in the first XMM-Newton observation, a sharp spectral drop is detected with energy that has shifted from 7 to 7.5 keV in two years. The drop is interpreted in terms of relativistically blurred ionized reflection from the a…

2004 Monthly Notices of the Royal Astronomical Society
XMM-Newton 160
The Local Lyα Forest. IV. Space Telescope Imaging Spectrograph G140M Spectra and Results on the Distribution and Baryon Content of H I Absorbers
DOI: 10.1086/382877 Bibcode: 2004ApJS..152...29P

Shull, J. Michael; Stocke, John T.; Penton, Steven V.

We present Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) G140M spectra of 15 extragalactic targets, which we combine with GHRS/G160M data to examine the statistical properties of the low-z Lyα forest. With STIS, we detect 109 Lyα absorbers at significance level (SL) of >=4 σ over 0.002<z<0.069, with a total reds…

2004 The Astrophysical Journal Supplement Series
eHST 157
Deflection of coronal mass ejection in the interplanetary medium
DOI: 10.1023/B:SOLA.0000043576.21942.aa Bibcode: 2004SoPh..222..329W

Wang, Yuming; Shen, Chenglong; Wang, S. +1 more

A solar coronal mass ejection (CME) is a large-scale eruption of plasma and magnetic fields from the Sun. It is believed to be the main source of strong interplanetary disturbances that may cause intense geomagnetic storms. However, not all front-side halo CMEs can encounter the Earth and produce geomagnetic storms. The longitude distribution of t…

2004 Solar Physics
SOHO 156