Search Publications

Tracking the energetics of the non-thermal disc-corona-jet in the very high state GX 339 - 4
DOI: 10.1093/mnras/stw585 Bibcode: 2016MNRAS.458.4238K

Done, C.; Kubota, A.

The dramatic hard-soft spectral transition in black hole binaries is important as it is associated with the collapse of the jet and with the strongest low-frequency quasi-periodic oscillations (QPOs). These transition spectra (intermediate and very high state: VHS) are complex, with soft but distinctly non-thermal Comptonization which merges smoot…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
Using radio stars to link the Gaia and VLBI reference frames
DOI: 10.1093/mnras/stw1488 Bibcode: 2016MNRAS.461.1937M

Malkin, Zinovy

A possible method for linking the optical Gaia Celestial Reference Frame (GCRF) to the VLBI-based International Celestial Reference Frame (ICRF) is to use radio stars in a manner similar to that in the linking of the Hipparcos Celestial Reference Frame (HCRF) to ICRF. In this work, an obtainable accuracy of the orientation angles between GCRF and …

2016 Monthly Notices of the Royal Astronomical Society
Gaia 12
Multi-spacecraft Analysis of Energetic Heavy Ion and Interplanetary Shock Properties in Energetic Storm Particle Events near 1 au
DOI: 10.3847/0004-637X/831/2/153 Bibcode: 2016ApJ...831..153E

Jian, L. K.; Mason, G. M.; Desai, M. I. +3 more

We examine the longitude distribution of and relationship between interplanetary (IP) shock properties and ∼0.1-20 MeV nucleon-1 O and Fe ions during seven multi-spacecraft energetic storm particle (ESP) events at 1 au. These ESP events were observed at two spacecraft and were primarily associated with low Mach number, quasi-perpendicul…

2016 The Astrophysical Journal
SOHO 12
Suzaku observations of the hard X-ray spectrum of Vela Jr. (SNR RX J0852.0-4622)
DOI: 10.1093/pasj/psw036 Bibcode: 2016PASJ...68S..10T

Katsuda, Satoru; Tashiro, Makoto S.; Terada, Yukikatsu +5 more

We report the results of Suzaku observations of the young supernova remnant, Vela Jr. (RX J0852.0-4622), which is known to emit synchrotron X-rays, as well as TeV gamma-rays. Utilizing 39 Suzaku mapping observation data from Vela Jr., a significant hard X-ray emission is detected with the hard X-ray detector (HXD) from the northwest TeV-emitting r…

2016 Publications of the Astronomical Society of Japan
Suzaku 12
Plasma observations during the Mars atmospheric "plume" event of March-April 2012
DOI: 10.1002/2015JA022023 Bibcode: 2016JGRA..121.3139A

Gurnett, D. A.; Barabash, S.; Holmström, M. +10 more

We present initial analyses and conclusions from plasma observations made during the reported "Mars plume event" of March-April 2012. During this period, multiple independent amateur observers detected a localized, high-altitude "plume" over the Martian dawn terminator, the cause of which remains to be explained. The estimated brightness of the pl…

2016 Journal of Geophysical Research (Space Physics)
MEx 12
Polarimetry of comets 67P/Churyumov-Gerasimenko, 74P/Smirnova-Chernykh, and 152P/Helin-Lawrence
DOI: 10.1051/0004-6361/201527696 Bibcode: 2016A&A...594A.110S

Jones, G. H.; Muinonen, K.; Protopapa, S. +5 more


Aims: Polarimetric characteristics of comets at large heliocentric distances is a relatively unexplored area; we extend the idea by adding and analysing the data for three Jupiter family comets (JFCs).
Methods: With the FORS2 instrument of the ESO VLT, we performed quasi-simultaneous photometry and polarimetry of three active JFCs 67P/Ch…

2016 Astronomy and Astrophysics
Rosetta 12
Analysis of the Herschel/Hexos Spectral Survey Toward Orion South: A Massive Protostellar Envelope with Strong External Irradiation
DOI: 10.3847/0004-637X/832/1/12 Bibcode: 2016ApJ...832...12T

Menten, K. M.; Pagani, L.; Lis, D. C. +14 more

We present results from a comprehensive submillimeter spectral survey toward the source Orion South, based on data obtained with the Heterodyne Instrument for the Far-Infrared instrument on board the Herschel Space Observatory, covering the frequency range of 480 to 1900 GHz. We detect 685 spectral lines with signal-to-noise ratios (S/Ns) > 3σ,…

2016 The Astrophysical Journal
Herschel 12
Analysis of a spatially deconvolved solar pore
DOI: 10.1093/mnras/stw1068 Bibcode: 2016MNRAS.460.1476Q

Ichimoto, K.; Suematsu, Y.; Katsukawa, Y. +3 more

Solar pores are active regions with large magnetic field strengths and apparent simple magnetic configurations. Their properties resemble the ones found for the sunspot umbra although pores do not show penumbra. Therefore, solar pores present themselves as an intriguing phenomenon that is not completely understood. We examine in this work a solar …

2016 Monthly Notices of the Royal Astronomical Society
Hinode 12
The Spitzer-IRAC/MIPS Extragalactic Survey (SIMES) in the South Ecliptic Pole Field
DOI: 10.3847/0067-0049/223/1/1 Bibcode: 2016ApJS..223....1B

Rodighiero, G.; Papovich, C.; Salvato, M. +25 more

We present the Spitzer-IRAC/MIPS Extragalactic survey (SIMES) in the South Ecliptic Pole field. The large area covered (7.7 deg2), together with one of the lowest Galactic cirrus emissions in the entire sky and a very extensive coverage by Spitzer, Herschel, Akari, and GALEX, make the SIMES field ideal for extragalactic studies. The elo…

2016 The Astrophysical Journal Supplement Series
Herschel 12
Isotopic ratio of nitrogen on Titan: Photochemical interpretation
DOI: 10.1016/j.pss.2016.10.008 Bibcode: 2016P&SS..134...61K

Krasnopolsky, Vladimir A.

Nitrogen isotope fractionation in predissociation of N2 (Liang et al., 2007) is combined with production of N(4S), N(2D), and N+ in dissociation and dissociative ionization by the solar EUV photons, photoelectrons, magnetospheric electrons and protons, and cosmic rays from the photochemical model. The ca…

2016 Planetary and Space Science
Cassini 12