Search Publications

Suzaku confirms NGC 3660 is an unabsorbed Seyfert 2
DOI: 10.1093/pasj/psv137 Bibcode: 2016PASJ...68S..24R

Nandra, Kirpal; Ueda, Yoshihiro; Bianchi, Stefano +3 more

An enigmatic group of objects, unabsorbed Seyfert 2s may have intrinsically weak broad line regions, obscuration in the line of sight to the BLR but not to the X-ray corona, or so much obscuration that the X-ray continuum is completely suppressed and the observed spectrum is actually scattered into the line of sight from nearby material. NGC 3660 …

2016 Publications of the Astronomical Society of Japan
Suzaku 1
Critical pitch angle for electron acceleration in a collisionless shock layer
DOI: 10.5194/angeo-34-591-2016 Bibcode: 2016AnGeo..34..591N

Narita, Y.; Motschmann, U.; Comişel, H.

Collisionless shock waves in space and astrophysical plasmas can accelerate electrons along the shock layer by an electrostatic potential, and scatter or reflect electrons back to the upstream region by the amplified magnetic field or turbulent fluctuations. The notion of the critical pitch angle is introduced for non-adiabatic electron accelerati…

2016 Annales Geophysicae
Cluster 1
Prometheus Induced Vorticity in Saturn's F Ring
DOI: 10.1007/s11038-016-9494-1 Bibcode: 2016EM&P..118..117S

Sutton, Phil J.; Kusmartsev, Feo V.

Saturn's rings are known to show remarkable real time variability in their structure. Many of which can be associated to interactions with nearby moons and moonlets. Possibly the most interesting and dynamic place in the rings, probably in the whole Solar System, is the F ring. A highly disrupted ring with large asymmetries both radially and azimu…

2016 Earth Moon and Planets
Cassini 1
The shape of Saturn's Huygens ringlet viewed by Cassini ISS
DOI: 10.1016/j.icarus.2016.04.035 Bibcode: 2016Icar..279..141S

Spitale, J. N.; Hahn, J. M.

A new model for the shape of the prominent eccentric ringlet in the gap exterior to Saturn's B ring is developed based on Cassini imaging observations taken over about 8 years. Unlike previous analyses, the new model treats each edge of the ringlet separately. The Keplerian component of the model is consistent with results derived from Voyager obs…

2016 Icarus
Cassini 1
Ultraviolet spectral variations of symbiotic nova PU Vul during and after second eclipse
DOI: 10.1007/s10509-016-2971-1 Bibcode: 2016Ap&SS.361..386S

Sanad, M. R.

I have analyzed spectral data of the symbiotic nova PU Vul observed with the International Ultraviolet Explorer (IUE) during the period 1993–1996. The study concentrated on the two sources of nebular emitting regions, the first is a nebula around the white dwarf partially eclipsed by a cool giant star and the second is a very extended nebular regi…

2016 Astrophysics and Space Science
IUE 1
The orbital phase resolved spectroscopy of X-ray binary 4U 1822-371 with Suzaku
DOI: 10.1088/1674-4527/16/4/057 Bibcode: 2016RAA....16...57N

Ji, Li; Nowak, Michael A.; Schulz, Norbert S. +3 more

4U 1822-371 is a typical edge-on eclipsing low mass X-ray binary and the prototype of accretion disk coronal sources. We report on the results of a spectral analysis over the energy range 0.5-45 keV observed by Suzaku in 2006. We extract spectra from five orbital phases. The spectra can be equally well described by various previously proposed mode…

2016 Research in Astronomy and Astrophysics
Suzaku 1
Cosmic rays from multi-wavelength observations of the Galactic diffuse emission
DOI: 10.1088/1742-6596/718/5/052027 Bibcode: 2016JPhCS.718e2027O

Orlando, Elena

Cosmic rays (CRs) generate diffuse emission while interacting with the Galactic magnetic field (B-field), the interstellar gas and the radiation field. This diffuse emission extends from radio, microwaves, through X-rays, to high-energy gamma rays. Diffuse emission has considerably increased the interest of the astrophysical community due to recen…

2016 Journal of Physics Conference Series
Planck 1
A Search for the Far-Infrared Ghost of C/2010 X1 (Elenin) with Herschel
DOI: 10.1007/s11038-016-9484-3 Bibcode: 2016EM&P..117..101K

Altieri, Bruno; Müller, Thomas; Kidger, Mark R. +1 more

Observations of Comet C/2010 X1 (Elenin) in August 2011 showed a pattern of evolution of coma morphology into an expanding, amorphous cloud of rapidly decreasing surface brightness shortly before perihelion passage, similar to C/1999 S4 (LINEAR) in 2000. However, the comet's difficult viewing geometry at the time of disruption made it impossible t…

2016 Earth Moon and Planets
Herschel 1
Rosetta mission: Space oddity
DOI: 10.1038/nphys3663 Bibcode: 2016NatPh..12..111G

Georgescu, Iulia

2016 Nature Physics
Rosetta 1
Identifying Surface Changes on HRSC Images of the Mars South Polar Residual CAP (sprc)
DOI: 10.5194/isprs-archives-XLI-B4-463-2016 Bibcode: 2016ISPAr41B4..463P

Muller, Jan-Peter; Putri, Alfiah Rizky Diana; Sidiropoulos, Panagiotis

The surface of Mars has been an object of interest for planetary research since the launch of Mariner 4 in 1964. Since then different cameras such as the Viking Visual Imaging Subsystem (VIS), Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC), and Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) and High Resolution Imaging Science Experim…

2016 ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences
MEx 1