Search Publications

Non-self-similar scaling of plasma sheet and solar wind probability distribution functions of magnetic field fluctuations
DOI: 10.1029/2006JA011820 Bibcode: 2006JGRA..11111209W

Balogh, A.; Khurana, K. K.; Kistler, L. M. +5 more

Solar wind magnetometer and plasma data and magnetometer data acquired by Cluster in the magnetospheric plasma sheet are employed to construct probability distribution functions (PDFs) of magnetic field fluctuations over various temporal and spatial scales. This technique, often used in analysis of laboratory plasmas, is used to look for intermitt…

2006 Journal of Geophysical Research (Space Physics)
Cluster 15
Adaptive-Optics-Assisted Near-Infrared Spectroscopy of SVS 13 and Its Jet
DOI: 10.1086/499557 Bibcode: 2006ApJ...639..969D

Smith, M. D.; Ray, T. P.; Nisini, B. +5 more

We present long-slit H- and K-band spectroscopy of the low-mass outflow source SVS 13, obtained with the adaptive-optics-assisted imager-spectrometer NACO on the VLT. With a spatial resolution of <0.25" and a pixel scale of 0.027", we precisely establish the relative offsets of H2, [Fe II], CO, H I, and Na I components from the sourc…

2006 The Astrophysical Journal
eHST 15
The Brave New World of Binary Star Studies
DOI: 10.1007/s10509-006-9069-0 Bibcode: 2006Ap&SS.304....5G

Guinan, Edward F.; Engle, Scott G.

In this paper we discuss some of the new and exciting developments in the study of binary stars. Recent technological advances (such as CCDs) now make it possible (even easy) to study faint, astrophysically important binaries that in the past could only be done with large 4 + meter class telescopes. Also, the panoramic nature of CCDs (and the use …

2006 Astrophysics and Space Science
eHST 15
INTEGRAL high energy behaviour of 4U 1812-12
DOI: 10.1051/0004-6361:20053917 Bibcode: 2006A&A...448..335T

Götz, D.; Capitanio, F.; Bird, A. J. +5 more

The low mass X-ray binary system 4U 1812-12 was monitored with the INTEGRAL observatory in the period 2003-2004 and with BeppoSAX on April 20, 2000. We report here on the spectral and temporal analysis of both persistent and burst emission. The full data set confirms the persistent nature of this burster, and reveals the presence of emission up to…

2006 Astronomy and Astrophysics
INTEGRAL 15
Statistical characteristics of hydrogen and oxygen ENA emission from the storm-time ring current
DOI: 10.1029/2005JA011201 Bibcode: 2006JGRA..111.6209O

Mitchell, D. G.; Roelof, E. C.; Brandt, P. C. +2 more

The present study statistically examines energetic neutral atom (ENA) emission from the storm-time inner magnetosphere using measurements from the IMAGE/HENA instrument. It is found that the total image-integrated ENA energy flux is well correlated (∣c.c.∣ ∼ 0.7) with the Sym-H index. However, the increase is not linear but exponential with ∣Sym-H…

2006 Journal of Geophysical Research (Space Physics)
Cassini 15
Host Galaxies of Two Micron All Sky Survey-selected QSOs at Redshift over 0.3
DOI: 10.1086/498725 Bibcode: 2006AJ....131..680H

Hutchings, J. B.; Cutri, R. M.; Cherniawsky, A. +1 more

We have obtained optical imaging with the Canada-France-Hawaii Telescope (CFHT) of 21 2MASS-selected QSOs of redshift greater than 0.3. This paper complements the sample of lower redshift 2MASS QSOs previously published. The QSOs have higher overall and nuclear luminosity, bluer colors, and higher ratio of nuclear to host flux than the lower redsh…

2006 The Astronomical Journal
eHST 15
The messy environment of Mrk 6
DOI: 10.1111/j.1365-2966.2006.10581.x Bibcode: 2006MNRAS.371..211S

Schurch, N. J.; Warwick, R. S.; Griffiths, R. E.

In recent years it has become clear that understanding the absorption present in active galactic nuclei (AGN) is essential given its bearing on unification models. We present the most recent XMM-Newton observation of Mrk 6, with the goal of understanding the nature and origin of the complex absorption intrinsic to this source. X-ray spectral fitti…

2006 Monthly Notices of the Royal Astronomical Society
XMM-Newton 15
Cluster observations in the magnetosheath - Part 2: Intensity of the turbulence at electron scales
DOI: 10.5194/angeo-24-3523-2006 Bibcode: 2006AnGeo..24.3523L

Maksimovic, M.; Trávníček, P.; Cornilleau-Wehrlin, N. +5 more

The Cluster STAFF Spectral Analyser measures the magnetic and electric power spectral densities (PSD) δB2 and δE2 in the magnetosheath between 8 Hz and 4 kHz, i.e. between about the lower hybrid frequency and 10 times the proton plasma frequency. We study about 23 h of data on four different days. We do not consider the whist…

2006 Annales Geophysicae
Cluster 15
An Atlas of Hubble Space Telescope STIS Spectra of Seyfert Galaxies
DOI: 10.1086/505910 Bibcode: 2006ApJS..166..498S

Calzetti, D.; Storchi-Bergmann, T.; Brandt, C. H. +1 more

We present a compilation of spectra of 101 Seyfert galaxies obtained with the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS), covering the UV and/or optical spectral range. Information on all the available spectra have been collected in a Mastertable, which is a very useful tool for anyone interested in a quick glance at …

2006 The Astrophysical Journal Supplement Series
eHST 15
Kinematics of O-B5 giants
DOI: 10.1111/j.1365-2966.2006.10582.x Bibcode: 2006MNRAS.370.1393B

Branham, Richard L.

To study the kinematics of O-B5 giant stars (luminosity class III), 290 non-Gould belt stars with proper motions taken from the Hipparcos catalogue are used, of which 107 have radial velocities taken from other sources. Semidefinite programming solves for the kinematical parameters and the coefficients of the velocity ellipsoid. The condition that…

2006 Monthly Notices of the Royal Astronomical Society
Hipparcos 15