Search Publications

The Interstellar Heliopause Probe/Heliospheric Explorer: IHP/HEX
DOI: 10.1063/1.3395952 Bibcode: 2010AIPC.1216..655W

Wimmer-Schweingruber, Robert F.; McNutt, Ralph L.

The Sun, driving a supersonic solar wind, cuts out of the local interstellar medium a giant plasma bubble, the heliosphere. Dedicated deep-space missions have greatly enhanced our understanding of our immediate neighborhood. Ulysses is the only spacecraft exploring the third, out-of-ecliptic dimension, while SOHO has allowed us to better understan…

2010 Twelfth International Solar Wind Conference
Ulysses 0
Geometry of Coronal Mass Ejections in the Context of Recent Solar Cycle
DOI: 10.2478/v10047-010-0004-3 Bibcode: 2010LatJP..47...64M

Mishra, Rajesh K.; Agarwal, Rekha

Coronal mass ejections (CMEs) disrupt the flow of the solar wind and produce disturbances that strike the Earth with sometimes catastrophic results. These ejections are often associated with solar flares and prominence eruptions, but they can also occur in the absence of either of these processes. The frequency of CMEs varies with the sunspot cycl…

2010 Latvian Journal of Physics and Technical Sciences
SOHO 0
INTEGRAL long-term monitoring results on persistently bright NS LMXBs
DOI: 10.1063/1.3475203 Bibcode: 2010AIPC.1248..199S

Kuulkers, E.; Farinelli, R.; Paizis, A. +3 more

We present long-term spectral and timing results from an INTEGRAL monitoring program of persistently bright neutron star Low-Mass X-ray Binaries, i.e. the three bright Atoll sources GX 3+1, GX 9+1 and GX 9+9, and the Z sources GX 5-1, GX 17+2, GX 340+0 and GX 349+2. From the available observing periods between 2003 and 2009, each lasting ~2 months…

2010 X-ray Astronomy 2009; Present Status, Multi-Wavelength Approach and Future Perspectives
INTEGRAL 0
Observational results from active region seismology
DOI: 10.1002/asna.201011427 Bibcode: 2010AN....331..920G

González Hernández, I.

Active regions are one of the most observed features in the solar surface. High-resolution solar telescopes on ground and space have revealed the fine configuration of umbra and penumbra of sunspots with amazing detail. However, the subsurface structure of sunspots and active regions remains, for the most part, unknown. Thanks to the development o…

2010 Astronomische Nachrichten
SOHO 0
Infrared limb sounding of Titan with the Cassini Composite InfraRed Spectrometer: effects of the mid-IR detector spatial responses: errata
DOI: 10.1364/AO.49.005575 Bibcode: 2010ApOpt..49.5575N

Nixon, Conor A.; Irwin, Patrick G. J.; Flasar, F. Michael +8 more

2010 Applied Optics
Cassini 0
Spectral Observations of AB Aur
Bibcode: 2010OAP....23...49I

Ismailov, N. Z.; Khalilov, O. V.

Results of spectral observations of the Herbig Ae/Be type star AB Aur carried out for 2008 - 2009 in SHAO were presented. The absorption component of the Hα line has a negative variable dis placement on different dates, reaching -300 km/s. To this absorption component superimposed an emission peak, which is rather unstable and can disappear com pl…

2010 Odessa Astronomical Publications
IUE 0
The Young Stellar Population of the Nearby Late-type Galaxy NGC 1311
DOI: 10.1088/0004-6256/140/5/1137 Bibcode: 2010AJ....140.1137E

Windhorst, Rogier A.; Eskridge, Paul B.; Jansen, Rolf A. +1 more

We have extracted point-spread-function-fitted stellar photometry from near-ultraviolet, optical, and near-infrared images, obtained with the Hubble Space Telescope, of the nearby (D ≈ 5.5 Mpc) SBm galaxy NGC 1311. The ultraviolet and optical data reveal a population of hot main-sequence (MS) stars with ages of 2-10 Myr. We also find populations o…

2010 The Astronomical Journal
eHST 0
Acceleration of >40 keV Electrons in Near-Earth Magnetotail Reconnection Events
DOI: 10.1007/978-90-481-3499-1_33 Bibcode: 2010ASSP...11..461A

Taylor, M. G. G. T.; Åsnes, A.; Borg, A. L.

Reconnection of magnetic field lines have been invoked as an acceleration mechanism producing significant amounts of super-thermal electrons in the high energy range. However, in a recent paper by Åsnes et al., 2008, energetic particle generation during geomagnetic active times was shown to be mainly caused by plasma sheet heating rather than reco…

2010 The Cluster Active Archive
Cluster 0
Planetary science: The birth of Saturn's baby moons
DOI: 10.1038/465701b Bibcode: 2010Natur.465..701B

Burns, Joseph A.

Simulations show that Saturn's nearby moons, after forming on the outskirts of the planet's main rings, get pushed clear of them. This model reproduces the moons' orbital locations and remarkably low densities.

2010 Nature
Cassini 0
The INTEGRAL Complete Sample of Type 1 AGN
DOI: 10.1063/1.3475309 Bibcode: 2010AIPC.1248..479M

Molina, M.

We present the average properties of a complete sample of 36 type 1 AGN, detected by INTEGRAL in the 20-40 keV band. We discuss the distribution of photon indices, high-energy cut-offs, reflection fractions and absorption properties and analyse their parameter space. We also investigate how our results fit into current frameworks for AGN spectral …

2010 X-ray Astronomy 2009; Present Status, Multi-Wavelength Approach and Future Perspectives
INTEGRAL 0