Search Publications

Near- to mid-infrared spectroscopy of the heavily obscured AGN LEDA 1712304 with AKARI/IRC
DOI: 10.1051/0004-6361/201935483 Bibcode: 2019A&A...626A.130T

Oyabu, S.; Toba, Y.; Kaneda, H. +5 more

Context. Although heavily obscured active galactic nuclei (AGNs) have been found by many observational studies, the properties of the surrounding dust are poorly understood. Using AKARI/IRC spectroscopy, we discovered a new heavily obscured AGN in LEDA 1712304 which shows a deep spectral absorption feature due to silicate dust.
Aims: We study…

2019 Astronomy and Astrophysics
AKARI Herschel 2
A Photometric Study of the Contact Binary V384 Serpentis
Bibcode: 2019JAVSO..47...43M

Michaels, E. J.; Lanning, C. M.; Self, S. N.

In this paper we present the first photometric light curves in the Sloan g', r', and i' passbands for the contact binary V384 Ser. Photometric solutions were obtained using the Wilson-Devinney program which revealed the star to be a W-type system with a mass ratio of q = 2.65 and a f = 36% degree of contact. The less massive component was found to…

2019 Journal of the American Association of Variable Star Observers (JAAVSO)
Gaia 2
An XMM-Newton look at the strongly variable radio-weak BL Lac Fermi J1544-0639
DOI: 10.1051/0004-6361/201834662 Bibcode: 2019A&A...622A.116U

Pian, E.; Masetti, N.; Ubertini, P. +6 more

Context. Fermi J1544-0639/ASASSN-17gs/AT2017egv was identified as a gamma-ray/optical transient on May 15, 2017. Subsequent multiwavelength observations suggest that this source may belong to the new class of radio-weak BL Lacs.
Aims: We studied the X-ray spectral properties and short-term variability of Fermi J1544-0639 to constrain the X-ra…

2019 Astronomy and Astrophysics
XMM-Newton 2
Generalized Additive Modeling Combined With Multiple Collinear for ICME Velocity Forecasting
DOI: 10.1029/2018SW002135 Bibcode: 2019SpWea..17..567L

Ji, H. S.; Wang, M.; Lu, J. Y. +5 more

One of the main issues of space weather is the timely prediction of disturbed solar wind parameters at L1, especially caused by Coronal Mass Ejection (CME). Using the data from 170 front halo, flare-associated CMEs, and in-site solar wind data, an analysis of the Interplanetary Coronal Mass Ejection (ICME) peak velocity at L1 related to associated…

2019 Space Weather
SOHO 2
Ultraviolet HST Spectroscopy of Planck Cold Clumps
DOI: 10.3847/1538-4357/aaff5d Bibcode: 2019ApJ...872..140D

Meyer, David M.; Dirks, Cody

We report results of the first study utilizing the ultraviolet capabilities of the Hubble Space Telescope to investigate a sample of Planck Galactic Cold Clump (PGCC) sources. We have selected high-resolution spectra toward 25 stars that contain a multitude of interstellar absorption lines associated with the interstellar medium (ISM) gas within t…

2019 The Astrophysical Journal
Gaia eHST 2
Kinematics of Hot Subdwarfs from the Gaia DR2 Catalogue
DOI: 10.1134/S1063773719080012 Bibcode: 2019AstL...45..580B

Bobylev, V. V.; Bajkova, A. T.

We have studied the kinematic properties of the candidates for hot subdwarfs (HSDs) selected by Geier et al. from theGaiaDR2 catalogue. We have used a total of 12 515 stars with relative trigonometric parallax errors less than 30%. The HSDs are shown to have different kinematics, depending on their positions on the celestial sphere. For example, t…

2019 Astronomy Letters
Gaia 2
Active experiments beyond the Earth: Plasma effects of sounding radar operations in the ionospheres of Venus, Mars, and the Jovian system
DOI: 10.3389/fspas.2019.00017 Bibcode: 2019FrASS...6...17V

Barabash, Stas; Holmstrom, Mats; Frahm, Rudy A. +1 more

Operation of powerful satellite- and rocket-born sounding radars is often accompanied by a heating/acceleration of the local electrons and ions. Intense fluxes of sounder accelerated particles were detected in Earth's ionosphere when the frequency of the radar transmitter was close to one of the fundamental plasma resonances: harmonic of the elect…

2019 Frontiers in Astronomy and Space Sciences
MEx VenusExpress 2
Seismological Determination of the Alfvén Speed and Plasma Beta in Solar Photospheric Bright Points
DOI: 10.3847/2041-8213/aafe0a Bibcode: 2019ApJ...871L..14C

Moon, Yong-Jae; Cho, Kyung-Suk; Kim, Yeon-Han +7 more

The Alfvén speed and plasma beta in photospheric bright points (BPs) observed by the Broadband Filter Imager (BFI) of the Solar Optical Telescope on board the Hinode satellite are estimated seismologically. The diagnostics is based on the theory of slow magnetoacoustic waves in a non-isothermally stratified photosphere with a uniform vertical magn…

2019 The Astrophysical Journal
Hinode 2
Formation of Central Pits in Impact Craters on Mars: A Statistical Investigation of Proposed Mechanisms
DOI: 10.1029/2018JE005738 Bibcode: 2019JGRE..124..437P

Burr, Devon M.; Peel, Samantha E.; Tran, Liem

Central pit craters (CPCs) are complex craters that exhibit depressions within their floors or central uplifts. Some proposed models for central pit formation can be grouped by similar mechanism: (A) explosive volatile release, (B) central peak collapse, and (C) drainage of subsurface melted volatiles. We test these groups of mechanisms for centra…

2019 Journal of Geophysical Research (Planets)
MEx 2
Isolated High-Density Structures in Magnetic Anomaly Regions of the Martian Lower Ionosphere
DOI: 10.1029/2018JA026400 Bibcode: 2019JGRA..124.6296M

Venkateswara Rao, N.; Leelavathi, V.; Mohanamanasa, P. +1 more

The occurrence of density structures in magnetic anomaly regions is one of the prominent features of the Martian ionosphere. These structures, in general, occur at altitudes above the main peak. In the present study, we analyze four cases of unusually strong oblique echoes that occur in magnetic anomaly regions and are observed by the Mars Express…

2019 Journal of Geophysical Research (Space Physics)
MEx 2