Search Publications

The Ringed Spiral Galaxy NGC4622. II. An Independent Determination that the Two Outer Arms Lead
DOI: 10.1088/0004-6256/135/1/408 Bibcode: 2008AJ....135..408B

Byrd, Gene G.; Freeman, Tarsh; Buta, Ronald J. +1 more

The spiral galaxy NGC4622 was recognized by Byrd et al. (1989, Celest. Mech., 45, 31) to have a single inner arm winding outward counterclockwise (CCW) and an outer pair of arms winding outward clockwise (CW). Using HST and ground-based observations, Buta et al. (2003, AJ, 125, 634) used a dust silhouette method to determine that the disk of NGC46…

2008 The Astronomical Journal
eHST 6
The Curlometer and Other Gradient Based Methods
Bibcode: 2008ISSIR...8...17D

Eastwood, Jonathan P.; Dunlop, Malcolm W.

The magnetic field measurements on the four Cluster spacecraft can be combined to produce a determination of the electric current density, j, point by point in time, from Ampere's law, i.e., through an estimate of the curl of the magnetic field, B, assuming the displacement current may be neglected (an assumption nearly always true in space plasma…

2008 ISSI Scientific Reports Series
Cluster 6
Ground-based variability surveys towards Centaurus A: worthwhile or not?
DOI: 10.1051/0004-6361:20078378 Bibcode: 2008A&A...478..755D

Héraudeau, P.; de Jong, J. T. A.; Kuijken, K. H.

Context: Difference imaging has proven to be a powerful technique for detecting and monitoring the variability of unresolved stellar sources in M 31. Using this technique in surveys of galaxies outside the Local Group could have many interesting applications.
Aims: The goal of this paper is to test difference imaging photometry on Centaurus A,…

2008 Astronomy and Astrophysics
eHST 6
Radiance and Doppler shift distributions across the network of the quiet Sun
DOI: 10.1051/0004-6361:200809923 Bibcode: 2008A&A...489.1297T

Tu, C. -Y.; Tian, H.; He, J. -S. +1 more

Aims: The radiance and Doppler-shift distributions across the solar network provide observational constraints of two-dimensional modeling of transition-region emission and flows in coronal funnels. These distributions have not, however, been studied in detail and we attempt an investigation for a quiet Sun region.
Methods: Two different method…

2008 Astronomy and Astrophysics
SOHO 6
Orientation of the hipparcos frame with respect to the reference frames of the DE403/LE403 and DE405/LE405 ephemerides based on asteroid observations
DOI: 10.1134/S1063773708040063 Bibcode: 2008AstL...34..266C

Chernetenko, Yu. A.

Highly accurate observations of 116 asteroids are used to determine the orientation of the Hipparcos frame with respect to the reference frames of the DE403/LE403 and DE405/LE405 majorplanet ephemerides. These observations include the photographic observations of 15 asteroids obtained as part of the programs for observing selected asteroids and re…

2008 Astronomy Letters
Hipparcos 6
The complex galaxy cluster Abell 514: New results obtained with the XMM-Newton satellite
DOI: 10.1051/0004-6361:20079289 Bibcode: 2008A&A...490..537W

Schindler, S.; Gitti, M.; Dolag, K. +1 more

Aims: We study the X-ray morphology and dynamics of the galaxy cluster Abell 514. Also, the relation between the X-ray properties and Faraday Rotation measures of this cluster are investigated in order to study the connection of magnetic fields and the intra-cluster medium.
Methods: We use two combined XMM-Newton pointings that are split into …

2008 Astronomy and Astrophysics
XMM-Newton 6
A Systematic Survey of H I Lyα and O VI Doublet Profiles Observed in Polar Coronal Holes at Solar Minimum
DOI: 10.1086/524885 Bibcode: 2008ApJ...674.1167N

Nakagawa, Akinari

A systematic, comprehensive survey of H I Lyα and O VI doublet profiles in polar coronal holes is performed using spectroscopic observation by the SOHO Ultraviolet Coronagraph Spectrometer (UVCS) at solar minimum in 1996-1997. By decomposing coronal hole profiles into component Gaussians, we determine detailed height distributions of profile param…

2008 The Astrophysical Journal
SOHO 6
The unusual UV continuum of quasar Ton 34 and the possibility of crystalline dust absorption
DOI: 10.1051/0004-6361:20078176 Bibcode: 2008A&A...478..739B

Binette, L.; Krongold, Y.

Context: Luminous quasars are known to display a sharp steepening of the continuum near 1100 Å. This spectral feature is not well fitted by current accretion disk models, unless Comptonization of the disk emission is invoked. Absorption by carbon crystalline dust has been proposed to account for this feature.
Aims: Ton 34 (zq = 1.92…

2008 Astronomy and Astrophysics
IUE eHST 6
Dissecting the star formation history of starburst galaxies: the case of NGC 7673
DOI: 10.1111/j.1365-2966.2008.12887.x Bibcode: 2008MNRAS.385..468P

Pasquali, A.; Castangia, P.

We have collected archival data on NGC 7673 to constrain the star formation history that produced the young star clusters and the field stellar population in this galaxy during the last 2 Gyr. We have considered the sample of 50 star clusters detected by Hubble Space Telescope/WFPC2 in the UV,V and I bands and estimated their age, intrinsic redden…

2008 Monthly Notices of the Royal Astronomical Society
IUE eHST 6
The infrared spectral features of circumstellar envelope of evolved low- and intermediate-mass stars
DOI: 10.1007/s11433-008-0136-0 Bibcode: 2008ScChG..51.1187Z

Zhang, Ke; Jiang, Biwei

The circumstellar envelope of evolved stars of low- and intermediate-mass is an important site for dust formation. In comparison with the interstellar medium, they have more types of organics and different types of inorganics. Various infrared features in the circumstellar envelope can reveal the composition and abundance of dust, as well as the c…

2008 Science in China: Physics, Mechanics and Astronomy
ISO 5