Search Publications

The Unusual Galactic Center Radio Source N3
DOI: 10.3847/0004-637X/826/2/218 Bibcode: 2016ApJ...826..218L

Morris, M. R.; Mills, E. A. C.; Mutel, R. +4 more

Here, we report on new multi-wavelength radio observations of the unusual point source “N3” that appears to be located in the vicinity of the Galactic Center (GC). VLA observations between 2 and 50 GHz reveal that N3 is a compact and bright source (56 mJy at 10 GHz) with a non-thermal spectrum superimposed upon the non-thermal radio filaments (NTF…

2016 The Astrophysical Journal
eHST 12
Testing the Effects of Expansion on Solar Wind Turbulence
DOI: 10.3847/2041-8205/832/1/L16 Bibcode: 2016ApJ...832L..16V

Chen, Christopher H. K.; Vech, Daniel

We present a multi-spacecraft approach to test the predictions of recent studies on the effect of solar wind expansion on the radial spectral, variance, and local 3D anisotropies of the turbulence. We found that on small scales (5000-10,000 km) the power levels of the B-trace structure functions do not depend on the sampling direction with respect…

2016 The Astrophysical Journal
Cluster 12
Preferred axis of CMB parity asymmetry in the masked maps
DOI: 10.1016/j.physletb.2016.04.030 Bibcode: 2016PhLB..757..445C

Cheng, Cheng; Huang, Qing-Guo; Santos, Larissa +1 more

Both WMAP and Planck data show a significant odd-multipole preference in the large scales of the cosmic microwave background (CMB) temperature anisotropies. If this pattern originates from cosmological effects, then it can be considered a crucial clue for a violation in the cosmological principle. By defining various direction dependent statistics…

2016 Physics Letters B
Planck 12
Suzaku follow-up of heavily obscured active galactic nuclei detected in Swift/BAT survey: NGC 1106, UGC 03752, and NGC 2788A
DOI: 10.1093/pasj/psw008 Bibcode: 2016PASJ...68S..26T

Tanimoto, Atsushi; Ueda, Yoshihiro; Kawamuro, Taiki +1 more

We present the broad-band (0.5-100 keV) spectra of three heavily obscured active galactic nuclei (AGNs), NGC 1106, UGC 03752, and NGC 2788A, observed with Suzaku and the Swift/Burst Alert Telescope (BAT). The targets are selected from the Swift/BAT 70-month catalog on the basis of their high hardness ratio between above and below 10 keV, and their…

2016 Publications of the Astronomical Society of Japan
Suzaku 12
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