Search Publications

A Steady, Radiative-Shock Method for Computing X-Ray Emission from Colliding Stellar Winds in Close, Massive-Star Binaries
DOI: 10.1086/422093 Bibcode: 2004ApJ...611..434A

Owocki, S. P.; Antokhin, I. I.; Brown, J. C.

We present a practical, efficient, semianalytic formalism for computing steady state X-ray emission from radiative shocks between colliding stellar winds in relatively close (orbital period up to order tens of days) massive-star, binary systems. Our simplified approach idealizes the individual wind flows as smooth and steady, ignoring the intrinsi…

2004 The Astrophysical Journal
XMM-Newton 85
Partial Covering Interpretation of the X-Ray Spectrum of the NLS1 1H 0707-495
DOI: 10.1093/pasj/56.3.L9 Bibcode: 2004PASJ...56L...9T

Ueda, Yoshihiro; Tanaka, Yasuo; Gallo, Luigi +2 more

The X-ray spectrum of 1H 0707 - 495 obtained with XMM-Newton showing a deep flux drop at ∼ 7 keV (Boller et al. 2002) is studied based on the partial covering concept. The previously inferred extreme iron overabundance can be reduced down to ∼ 3× solar if the hard component gradually steepens at high energies. The spectral shape supports that 1H 0…

2004 Publications of the Astronomical Society of Japan
XMM-Newton 85
Anatomy of a flux transfer event seen by Cluster
DOI: 10.1029/2004GL020134 Bibcode: 2004GeoRL..3111803S

Hasegawa, H.; Paschmann, G.; Sonnerup, B. U. Ö.

Data from Cluster are used to study the structure of a flux transfer event (FTE), seen near the northern cusp. We employ Grad-Shafranov reconstruction, using measured fields from all four spacecraft to produce a map of the FTE cross section. The FTE consists of a flux rope of approximate size 1RE and irregular shape, embedded in the mag…

2004 Geophysical Research Letters
Cluster 85
RR Lyrae Stars in the Andromeda Halo from Deep Imaging with the Advanced Camera for Surveys
DOI: 10.1086/386355 Bibcode: 2004AJ....127.2738B

Ferguson, Henry C.; Brown, Thomas M.; Rich, R. Michael +4 more

We present a complete census of RR Lyrae stars in a halo field of the Andromeda galaxy. These deep observations, taken as part of a program to measure the star formation history in the halo, spanned a period of 41 days with sampling on a variety of timescales, enabling the identification of short- and long-period variables. Although the long-perio…

2004 The Astronomical Journal
eHST 85
The ACS Virgo Cluster Survey. II. Data Reduction Procedures
DOI: 10.1086/422977 Bibcode: 2004ApJS..154..509J

Jordán, Andrés; Tonry, John L.; Côté, Patrick +7 more

The ACS Virgo Cluster Survey is a large program to carry out multicolor imaging of 100 early-type members of the Virgo Cluster using the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope. Deep F475W and F850LP images (~SDSS g and z) are being used to study the central regions of the program galaxies, their globular cluster systems, a…

2004 The Astrophysical Journal Supplement Series
eHST 84
Coronal Mass Ejection of 15 May 2001: II. Coupling of the Cme Acceleration and the Flare Energy Release
DOI: 10.1007/s11207-004-4995-x Bibcode: 2004SoPh..225..355V

Maričić, D.; Vršnak, B.; Stanger, A. L. +1 more

We analyze the relationship between the dynamics of the coronal mass ejection (CME) of 15 May 2001 and the energy release in the associated flare. The flare took place behind the east limb and was disclosed by a growing system of hot soft X-ray (SXR) loops that appeared from behind the limb around the onset of the rapid acceleration of the CME. Th…

2004 Solar Physics
SOHO 84
Mapping the inner regions of MCG-6-30-15 with XMM-Newton
DOI: 10.1051/0004-6361:20031758 Bibcode: 2004A&A...417..451P

Cappi, M.; Ponti, G.; Dadina, M. +1 more

Timing analysis of a ∼95 ks long XMM-Newton observation of the Seyfert 1 galaxy MCG-6-30-15 is presented. Model-independent tools have been used with the intent of resolving the different components that produce the observed flux and spectral variations down to timescales as short as ∼300 s. We find that the fractional variability is possibly due …

2004 Astronomy and Astrophysics
XMM-Newton 84
X-Ray Sources and Their Optical Counterparts in the Globular Cluster M4
DOI: 10.1086/421259 Bibcode: 2004ApJ...609..755B

Anderson, Scott F.; Kaspi, Victoria M.; Verbunt, Frank +7 more

We report on the Chandra X-Ray Observatory ACIS-S3 imaging observation of the Galactic globular cluster M4 (NGC 6121). We detect 12 X-ray sources inside the core and 19 more within the cluster half-mass radius. The limiting luminosity of this observation is LX~1029 ergs s-1 for sources associated with the cluster, …

2004 The Astrophysical Journal
eHST 84
Solar and Heliospheric Phenomena in October-November 2003: Causes and Effects
DOI: 10.1023/B:COSM.0000046229.24716.02 Bibcode: 2004CosRe..42..435V

Petrukovich, A. A.; Zelenyi, L. M.; Yermolaev, Yu. I. +72 more

We present new observational data on the phenomena of extremely high activity on the Sun and in the heliosphere that took place in October-November 2003. A large variety of solar and heliospheric parameters give evidence that the interval under consideration is unique over the entire observation time. Based on these data, comparing them with simil…

2004 Cosmic Research
SOHO 84
The Solar Neighborhood. IX. Hubble Space Telescope Detections of Companions to Five M and L Dwarfs within 10 Parsecs of the Sun
DOI: 10.1086/423911 Bibcode: 2004AJ....128.1733G

Illingworth, Garth D.; Nelan, Edmund P.; Ardila, David R. +10 more

We report the detections of low-mass companions to five M and L dwarfs within 10 pc of the Sun using the Hubble Space Telescope (HST) Near-Infrared Camera and Multi-Object Spectrometer (NICMOS). Follow-up observations using the HST Advanced Camera for Surveys (ACS) and Fine Guidance Sensor 1r (FGS1r) confirm our NICMOS discoveries of companions to…

2004 The Astronomical Journal
eHST 84