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AKARI Infrared Camera Survey of the Large Magellanic Cloud
DOI: 10.5303/PKAS.2017.32.1.083 Bibcode: 2017PKAS...32...83S

Onaka, T.; Ita, Y.; Kato, D. +2 more

We conducted an unbiased near- to mid-infrared imaging and spectroscopic survey of the Large Magellanic Cloud (LMC) as a part of the AKARI Mission Program "Large-area Survey of the LMC" (LSLMC, PI: T. Onaka). An area of about 10 square degrees of the LMC was observed by five photometric bands (3.2, 7, 11, 15, and 24 µm) and a low-resolution …

2017 Publication of Korean Astronomical Society
AKARI 0
Dawn-Dusk Asymmetries of Ionospheric Outflow
DOI: 10.1002/9781119216346.ch21 Bibcode: 2017GMS...230..273L

Wei, Y.; Daly, P. W.; André, M. +3 more

2017 Dawn-Dusk Asymmetries in Planetary Plasma Environments
Cluster 0
Unveiling the physics of AGN through X-ray variability
Bibcode: 2017hsa9.conf..169H

González-Martín, O.; Márquez, I.; Masegosa, J. +1 more

Although variability is a general property characterizing active galactic nuclei (AGN), it is not well established whether the changes occur in the same way in every nuclei. The main purpose of this work is to study the X-ray variability pattern(s) in AGN selected at optical wavelengths in a large sample, including low ionization nuclear emission …

2017 Highlights on Spanish Astrophysics IX
XMM-Newton 0
IR photometry results and dust envelope model for symbiotic Mira star candidate V 335 Vul
DOI: 10.1134/S1990341317040071 Bibcode: 2017AstBu..72..447B

Bogdanov, M. B.; Taranova, O. G.; Shenavrin, V. I.

We present the results of JHKLM-photometry for the symbiotic Mira star candidate V 335 Vul. Based on the average flux data, supplemented by IRAS, MSX, AKARI, and WISE mid-IR observations, we calculated a model of a spherically symmetric dust envelope of the star, made up of amorphous carbon and silicon carbide particles. The optical depth of the e…

2017 Astrophysical Bulletin
AKARI 0
Akari-Nep : Effects of AGN Presence on SFR Estimates of Galaxies
DOI: 10.5303/PKAS.2017.32.1.239 Bibcode: 2017PKAS...32..239M

Berta, S.; Rodighiero, G.; White, G. J. +11 more

2017 Publication of Korean Astronomical Society
AKARI 0
Recursive Range Estimation Using Astrophysical Signals of Opportunity
DOI: 10.2514/1.G002650 Bibcode: 2017JGCD...40.2201R

Runnels, Joel T.; Gebre-Egziabher, Demoz

2017 Journal of Guidance Control Dynamics
Suzaku 0
Effects of the convective field on weakly outgassing comets
DOI: 10.1093/mnras/sty430 Bibcode: 2017MNRAS.469S.824B

Galand, M.; Beth, A.

By applying a kinetic approach, we have developed two models in order to assess the influence of one main driver of plasma acceleration, the convective electric field, on the cometary ion distribution at 67P/Churyumov-Gerasimenko (67P/C-G). This electric field is carried by the solar wind and corresponds to the acceleration undergone by cometary i…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 0
La poussiere cosmique
Bibcode: 2017LAstr.131f..22R

Rotundi, Alessandra

Since the 1970s, dust has been collected in the terrestrial environment in the hope of studying dust particles witnessing the primordial protoplanetary nebula materials. In the 21th century, cometary dust was collected by the Stardust/NASA probe in the coma of comet 81P/Wild-2 and returned to Earth. Cometary dust was also analyzed in situ by Roset…

2017 L'Astronomie
Rosetta 0
News on the X-ray emission from hot subdwarf stars
DOI: 10.1515/astro-2017-0435 Bibcode: 2017OAst...26..187P

Mereghetti, Sandro; Palombara, Nicola La

In latest years, the high sensitivity of the instruments on-board the XMM-Newton and Chandra satellites allowed us to explore the properties of the X-ray emission from hot subdwarf stars. The small but growing sample of X-ray detected hot subdwarfs includes binary systems, in which the X-ray emission is due to wind accretion onto a compact compani…

2017 Open Astronomy
XMM-Newton 0
The evolution of geomagnetotail magnetic flux in isolated substorms
DOI: 10.1016/j.jastp.2017.08.016 Bibcode: 2017JASTP.164..163Y

Dunlop, M.; Rong, Z. J.; Shen, C. +4 more

The magnetic field energy stored in geomagnetotail released during a substorm period, cause significant magnetic disturbance of the space environment. The quantitative relationship between the magnetic field energy and the level of substorm activity, however, is still unclear, although many studies have qualitatively revealed the correlation betwe…

2017 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 0