Search Publications

The interplay between active galactic nuclei and star formation activities of type 1 active galactic nuclei probed by polycyclic aromatic hydrocarbon 3.3 µm emission feature with AKARI
DOI: 10.1093/pasj/psy144 Bibcode: 2019PASJ...71...25K

Nakagawa, Takao; Oyabu, Shinki; Ohyama, Youichi +11 more

We investigate the connection between active galactic nucleus (AGN) and star formation activities of AGN host galaxies by studying the 3.3 µm polycyclic aromatic hydrocarbon (PAH) emission feature of 79 type 1 AGNs using the AKARI space telescope. Utilizing the slitless spectroscopic capability of the AKARI Infrared Camera, we obtained the s…

2019 Publications of the Astronomical Society of Japan
AKARI 4
X-ray activity from different types of stars
DOI: 10.1088/1674-4527/19/7/98 Bibcode: 2019RAA....19...98H

Zhang, Yong; Soria, Roberto; Bai, Yu +10 more

X-ray emission is an important indicator of stellar activity. In this paper, we study stellar X-ray activity using the XMM-Newton and LAMOST data for different types of stars. We provide a sample including 1259 X-ray-emitting stars, of which 1090 have accurate stellar parameter estimations. Our sample size is much larger than those used in previou…

2019 Research in Astronomy and Astrophysics
XMM-Newton 4
Warm CO in evolved stars from the THROES catalogue. II. Herschel/PACS spectroscopy of C-rich envelopes
DOI: 10.1051/0004-6361/201834141 Bibcode: 2019A&A...622A.123D

García-Lario, P.; Sánchez Contreras, C.; da Silva Santos, J. M. +1 more

Context. This is the second paper of a series making use of Herschel/PACS spectroscopy of evolved stars in the THROES catalogue to study the inner warm regions of their circumstellar envelopes (CSEs).
Aims: We analyse the CO emission spectra, including a large number of high-J CO lines (from J = 14-13 to J = 45-44, ν = 0), as a proxy for the …

2019 Astronomy and Astrophysics
Herschel 4
The loud and the quiet: searching for radio counterparts of two radio-weak BL Lac candidates with VLBI
DOI: 10.1093/mnrasl/sly184 Bibcode: 2019MNRAS.482L..34C

Frey, Sándor; Yang, Jun; An, Tao +4 more

BL Lac objects are known to have compact jets inclined to our line of sight at a small angle, showing prominent radio emission. Two radio-weak BL Lac candidates with no counterparts in current radio surveys were recently reported by Massaro et al. Both sources were selected as candidate low-energy counterparts of unassociated Fermi γ-ray sources. …

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
Signal enhancement for planetary radar sounders
DOI: 10.1049/el.2018.7284 Bibcode: 2019ElL....55..153P

Seu, R.; Mastrogiuseppe, M.; Piazzo, L. +1 more

2019 Electronics Letters
MEx 4
Geomorphological Evidence of Localized Stagnant Ice Deposits in Terra Cimmeria, Mars
DOI: 10.1029/2018JE005772 Bibcode: 2019JGRE..124.1525A

Hauber, Ernst; Jaumann, Ralf; Fawdon, Peter +3 more

The presence of snow and ice at midlatitudes of Mars cannot be explained by current climatic conditions, as surface ice is unstable. However, a large variety of debris-covered glaciers have been observed at both midlatitudes. Here, we report the presence of local, small-scale, and debris-covered stagnant ice deposits on the floor of a valley syste…

2019 Journal of Geophysical Research (Planets)
MEx 4
Variation of coronal holes latitudinal distribution: Correction of limb brightening of EUV coronal images
DOI: 10.1016/j.asr.2019.04.009 Bibcode: 2019AdSpR..64..491C

Chargeishvili, B. B.; Maghradze, D. A.; Japaridze, D. R. +4 more

We studied the limb brightening of SOHO EIT daily images of the solar corona taken in 195 Å wavelength line from 1996 to 2018. Using special software, we studied the distribution of the background intensity of the entire disk in the direction of rotation (horizontally) and perpendicular to the direction of rotation (vertical). The study shows that…

2019 Advances in Space Research
SOHO 4
2FHL J0826.1-4500: Discovery of a Possible Shock-Cloud Interaction on the Western Edge of the Vela Supernova Remnant
DOI: 10.3847/1538-4357/aaf0ff Bibcode: 2019ApJ...870...35E

Ajello, M.; Tibaldo, L.; Marchesi, S. +3 more

We report on the investigation of a very high-energy, Galactic γ-ray source recently discovered at >50 GeV using the Large Area Telescope on board Fermi. This object, 2FHL J0826.1-4500, displays one of the hardest >50 GeV spectra (photon index Γ γ ∼ 1.6) in the 2FHL catalog, and a follow-up observation with XMM-Newton has uncover…

2019 The Astrophysical Journal
XMM-Newton 4
HD 42659: the only known roAp star in a spectroscopic binary observed with B photometry, TESS, and SALT
DOI: 10.1093/mnras/stz2419 Bibcode: 2019MNRAS.489.4063H

Holdsworth, Daniel L.; Saio, Hideyuki; Kurtz, Donald W.

We present a multi-instrument analysis of the rapidly oscillating Ap (roAp) star HD 42659. We have obtained B photometric data for this star and use these data, in conjunction with the Transiting Exoplanet Survey Satellite (TESS) observations, to analyse the high-frequency pulsation in detail. We find a triplet that is split by the rotation freque…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 4
Post-rendezvous radar properties of comet 67P/CG from the Rosetta Mission: understanding future Earth-based radar observations and the dynamical evolution of comets
DOI: 10.1093/mnras/stz2174 Bibcode: 2019MNRAS.489.1667H

Kofman, Wlodek; Heggy, Essam; Palmer, Elizabeth M. +2 more

Radar observations provide crucial insights into the formation and dynamical evolution of comets. This ability is constrained by our knowledge of the dielectric and textural properties of these small-bodies. Using several observations by Rosetta as well as results from the Earth-based Arecibo radio telescope, we provide an updated and comprehensiv…

2019 Monthly Notices of the Royal Astronomical Society
Rosetta 4