Search Publications

Possible Precession Motion in the Bipolar Proto-Planetary Nebula IRAS 17441-2411
DOI: 10.1086/522225 Bibcode: 2007ApJ...670.1137V

Volk, Kevin; Kwok, Sun; Hrivnak, Bruce J.

Mid-infrared imaging of two bipolar proto-planetary nebulae, IRAS 17150-3224 and IRAS 17441-2411, was obtained with the Gemini telescope. Dust emissions are detected in both the bipolar lobes and in the equatorial region of IRAS 17441-2411. In particular, the orientation of the axis of the infrared torus is found to be offset by 23° from the bipol…

2007 The Astrophysical Journal
eHST 14
A precessing accretion disc in the intermediate polar XY Arietis?
DOI: 10.1051/0004-6361:20077761 Bibcode: 2007A&A...472..225N

Mukai, K.; Norton, A. J.

Context: XY Ari is the only intermediate polar to show deep X-ray eclipses of its white dwarf. Previously published observations with Ginga and Chandra have also revealed a broad X-ray orbital modulation, roughly antiphased with the eclipse, and presumed to be due to absorption in an extended structure near the edge of an accretion disc. The X-ray…

2007 Astronomy and Astrophysics
XMM-Newton 14
An ultraluminous supersoft source with a 4 hour modulation in NGC 4631
DOI: 10.1051/0004-6361:20077605 Bibcode: 2007A&A...471L..55C

Ehle, M.; Wilms, J.; King, A. R. +2 more

Context: Supersoft X-ray sources (SSSs) are characterised by very low temperatures (<100 eV). Classical SSSs have bolometric luminosities in the range of 1036-1038 erg s-1 and are modelled with steady nuclear burning of hydrogen on the surfaces of white dwarfs. However, several SSSs have been discovered with muc…

2007 Astronomy and Astrophysics
XMM-Newton 14
The Host Galaxies and Environment of Chandra-Selected Active Galactic Nuclei in the Deep ACS GTO Cluster Fields
DOI: 10.1086/509256 Bibcode: 2007ApJS..168...19M

Infante, Leopoldo; Tozzi, Paolo; Ford, Holland C. +2 more

We present catalogs and images of optical counterparts to the Chandra-selected X-ray sources found in the fields of the five clusters RX J0152-1357, RX J0849+4452, RDCS J0910+5422, MS 1054-0321, and RDCS J1252-2927, which were imaged with the Advanced Camera for Surveys as part of the ACS Guaranteed Time Observer programs. A total of 98 X-ray sour…

2007 The Astrophysical Journal Supplement Series
eHST 14
X-Ray and Ultraviolet Spectroscopy of Intermediate-Mass, First Crossing Giants
DOI: 10.1086/516713 Bibcode: 2007ApJS..171..304A

Ayres, Thomas R.; Brown, Alexander; Hodges-Kluck, Edmund

Chandra, FUSE, and HST STIS jointly have obtained spectra of four intermediate-mass giants (<~3 Msolar) crossing the Hertzsprung gap for the first time, passing through a ``rapid braking phase'' analogous to, but much briefer than, the more gradual prolonged decay of magnetic activity experienced by single low-mass stars like the Sun…

2007 The Astrophysical Journal Supplement Series
eHST 14
Emission heights of coronal bright points on Fe XII radiance map
DOI: 10.1016/j.asr.2007.03.065 Bibcode: 2007AdSpR..39.1853T

Tu, C. -Y.; Marsch, E.; Tian, H. +1 more

The study of coronal bright points (BPs) is important for understanding coronal heating and the origin of the solar wind. Previous studies indicated that coronal BPs have a highly significant tendency to coincide with magnetic neutral lines in the photosphere. Here we further studied the emission heights of the BPs above the photosphere in the bip…

2007 Advances in Space Research
SOHO 14
Analytical Models for Cross-Correlation Signal in Time-Distance Helioseismology
DOI: 10.1086/512535 Bibcode: 2007ApJ...659.1736N

Kosovichev, A. G.; Scherrer, P. H.; Nigam, R.

In time-distance helioseismology, the time signals (Doppler shifts) at two points on the solar surface separated by a fixed angular distance are cross-correlated, and this leads to a wave packet signal. Accurately measuring the travel times of these wave packets is crucial for inferring the subsurface properties in the Sun. The observed signal is …

2007 The Astrophysical Journal
SOHO 14
Two-Dimensional Spectroscopy of Photospheric Shear Flows in a Small δ Spot
DOI: 10.1007/s11207-007-9039-x Bibcode: 2007SoPh..245..219D

Yurchyshyn, V.; Tritschler, A.; Denker, C. +1 more

In recent high-resolution observations of complex active regions, long-lasting and well-defined regions of strong flows were identified in major flares and associated with bright kernels of visible, near-infrared, and X-ray radiation. These flows, which occurred in the proximity of the magnetic neutral line, significantly contributed to the genera…

2007 Solar Physics
SOHO 14
Submillimeter lightcurves of Vesta
DOI: 10.1016/j.icarus.2007.08.003 Bibcode: 2007Icar..192..448C

Sykes, Mark V.; Lovell, Amy J.; Chamberlain, Matthew A.

Thermal lightcurves of Asteroid Vesta with significant amplitude have been observed at 870 µm (345 GHz) using the MPIfR 19-channel bolometer of the Heinrich-Hertz Submillimeter Telescope. Shape and albedo are not sufficient to explain the magnitude of this variation, which we relate to global variations in thermal inertia and/or other thermo…

2007 Icarus
eHST 14
Dynamics of two satellites in the 2/1 Mean–Motion resonance: application to the case of Enceladus and Dione
DOI: 10.1007/s10569-007-9066-9 Bibcode: 2007CeMDA..98....5C

Yokoyama, T.; Callegari, N.

The dynamics of a pair of satellites similar to Enceladus–Dione is investigated with a two-degrees-of-freedom model written in the domain of the planar general three-body problem. Using surfaces of section and spectral analysis methods, we study the phase space of the system in terms of several parameters, including the most recent data. A detaile…

2007 Celestial Mechanics and Dynamical Astronomy
Cassini 14