Search Publications

Induced magnetosphere and its outer boundary at Venus
DOI: 10.1029/2008JE003215 Bibcode: 2008JGRE..113.0B20Z

Barabash, S.; Russell, C. T.; Wei, H. Y. +8 more

The induced magnetosphere at Venus consists of regions near the planet and its wake for which the magnetic pressure dominates all other pressure contributions. Initial Venus Express measurements indicate a well-defined outer boundary, the magnetopause, of the induced magnetosphere. This magnetopause acts as an obstacle to deflect the solar wind. A…

2008 Journal of Geophysical Research (Planets)
VenusExpress 46
Characterizing the Near-UV Environment of M Dwarfs
DOI: 10.1086/526421 Bibcode: 2008ApJ...677..593W

Hawley, Suzanne L.; Johns-Krull, Christopher M.; Walkowicz, Lucianne M.

We report the results of our Hubble Space Telescope (HST) snapshot survey with the ACS HRC PR200L prism, designed to measure the near-UV emission in a sample of nearby M dwarfs. Thirty-three stars were observed, spanning the mass range from 0.1 to 0.6 solar masses (Teff ~ 2200-4000 K) where the UV energy distributions vary widely betwee…

2008 The Astrophysical Journal
IUE eHST 46
High-Resolution Mapping of Flows in the Solar Interior: Fully Consistent OLA Inversion of Helioseismic Travel Times
DOI: 10.1007/s11207-008-9158-z Bibcode: 2008SoPh..251..381J

Birch, A. C.; Gizon, L.; Jackiewicz, J.

To recover the flow information encoded in travel-time data of time - distance helioseismology, accurate forward modeling and a robust inversion of the travel times are required. We accomplish this using three-dimensional finite-frequency travel-time sensitivity kernels for flows along with a (2+1)-dimensional (2+1D) optimally localized averaging …

2008 Solar Physics
SOHO 46
INTEGRAL discovery of non-thermal hard X-ray emission from the Ophiuchus cluster
DOI: 10.1051/0004-6361:20078853 Bibcode: 2008A&A...479...27E

Paltani, S.; Eckert, D.; Produit, N. +2 more

We present the results of deep observations of the Ophiuchus cluster of galaxies with INTEGRAL in the 3-80 keV band. We analyse 3 Ms of INTEGRAL data on the Ophiuchus cluster with the IBIS/ISGRI hard X-ray imager and the JEM-X X-ray monitor. In the X-ray band using JEM-X, we show that the source is extended, and that the morphology is compatible w…

2008 Astronomy and Astrophysics
INTEGRAL 46
High-latitude Earth's magnetopause outside the cusp: Cluster observations
DOI: 10.1029/2006JA012123 Bibcode: 2008JGRA..113.1220P

RèMe, H.; Korth, A.; Büchner, J. +4 more

We investigated the ambient plasma and magnetic field conditions at high latitudes, as well as the macroparameters of the magnetopause. For this purpose we used Cluster spacecraft plasma and magnetic field data when all the interspacecraft distances were less than 300 km. We analyzed 154 magnetosheath-magnetosphere transitions which allow to disti…

2008 Journal of Geophysical Research (Space Physics)
Cluster 46
INTEGRAL observations of the blazar Mrk 421 in outburst. Results of a multi-wavelength campaign
DOI: 10.1051/0004-6361:20079199 Bibcode: 2008A&A...486..721L

Lähteenmäki, A.; Ajello, M.; Horan, D. +15 more

Context: If one wants to understand the physics of blazars, better simultaneous observations are important at all wavelengths, so it was fortunate that a ToO observation of the TeV-emitting blazar Mrk 421 with INTEGRAL could be triggered in June 2006 by an increase in the RXTE count rate to more than 30 mCrab. The source was then observed with all…

2008 Astronomy and Astrophysics
INTEGRAL 46
Rotational Feature of Vega Revealed from Spectral Line Profiles
DOI: 10.1086/528949 Bibcode: 2008ApJ...678..446T

Takeda, Yoichi; Kawanomoto, Satoshi; Ohishi, Naoko

In order to establish Vega's absolute rotational velocity, ve, as distinct from the inclination angle, i, we conducted a detailed profile study on a large number (~200) of weak lines based on very high signal-to-noise ratio spectrum data, making use of the fact that the lines' characteristic shapes may contain information about rotation…

2008 The Astrophysical Journal
IUE eHST 46
Giant outburst of EXO 2030+375: pulse-phase resolved analysis of INTEGRAL data
DOI: 10.1051/0004-6361:200810673 Bibcode: 2008A&A...491..833K

Klochkov, D.; Santangelo, A.; Ferrigno, C. +1 more

In June-September 2006 the Be/X-ray binary EXO 2030+375 experienced the second giant outburst since its discovery. The source was shown to have a complicated pulse-averaged X-ray spectral continuum with possible evidence of cyclotron absorption features. In this paper we present the first pulse-phase resolved analysis of the broad band X-ray spect…

2008 Astronomy and Astrophysics
INTEGRAL 46
Investigation of water vapor on Mars with PFS/SW of Mars Express
DOI: 10.1016/j.icarus.2008.01.018 Bibcode: 2008Icar..195..557T

Lellouch, E.; Ignatiev, N. I.; Fouchet, T. +4 more

New insight into the seasonal, diurnal and spatial distribution of water vapor on Mars has been obtained from analyzing the spectra of the short-wavelength channel (SW) of the Planetary Fourier Spectrometer (PFS) onboard Mars Express. The processed dataset, recorded between January 2004 and April 2005, covers the seasons from L=331° of Mars Year 2…

2008 Icarus
MEx 46
Suzaku Wide-Band X-Ray Spectroscopy of the Seyfert2 AGN in NGC 4945
DOI: 10.1093/pasj/60.sp1.S251 Bibcode: 2008PASJ...60S.251I

Done, Chris; Isobe, Naoki; Gandhi, Poshak +13 more

Suzaku observed a nearby Seyfert2 galaxy, NGC 4945, which hosts one of the brightest active galactic nuclei above 20keV. Combining data from the two detectors aboard Suzaku, the AGN intrinsic nuclear emission and its reprocessed signals were observed simultaneously. The intrinsic emission is highly obscured with an absorbing column of ∼5×1024…

2008 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 46