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More planetary candidates from K2 Campaign 5 using TRAN_K2
DOI: 10.1051/0004-6361/202038726 Bibcode: 2020A&A...643A.169K

Kovacs, Geza

Context. The exquisite precision of space-based photometric surveys and the unavoidable presence of instrumental systematics and intrinsic stellar variability call for the development of sophisticated methods that distinguish these signal components from those caused by planetary transits.
Aims: Here, we introduce the standalone Fortran code …

2020 Astronomy and Astrophysics
Gaia 2
The characteristics of the coronal mass ejections preceding the associated X-ray and γ-ray burst solar flares
DOI: 10.1016/j.newast.2019.101285 Bibcode: 2020NewA...7401285M

Abdel-Sattar, Walid; Mawad, Ramy

In this study, investigated 14,786 coronal mass ejection (CME) events and 5092 Gamma-ray Burst Monitor (GBM) solar flare events (called γ-ray burst solar flare) recorded during 2008-2017, by using temporal and spatial conditions criteria, we found 845 (about 16%) CME events associated with γ-ray burst solar flare events only (hereafter, CME-γ-pref…

2020 New Astronomy
SOHO 2
IVOA HiPS implementation in the framework of WorldWide Telescope
DOI: 10.1016/j.ascom.2020.100380 Bibcode: 2020A&C....3100380X

Li, S.; Li, C.; Xu, Y. +9 more

The WorldWide Telescope(WWT) is a scientific visualization platform which can browse deep space images, star catalogs, and planetary remote sensing data from different observation facilities in a three-dimensional virtual scene. First launched and then open-sourced by Microsoft Research, the WWT is now managed by the American Astronomical Society …

2020 Astronomy and Computing
Gaia 2
[Rb/Zr] ratio in Ba stars as a diagnostic of the companion AGB stellar mass
DOI: 10.1007/s12036-020-09654-7 Bibcode: 2020JApA...41...37S

Shejeelammal, J.; Goswami, Aruna

Understanding nucleosynthesis in and evolution of asymptotic giant branch (AGB) stars is of primary importance as these stars are the main producers of some of the key elements in the Universe. They are the predominant sites for slow-neutron-capture nucleosynthesis (s-process). The exact physical conditions and nucleosynthetic processes occurring …

2020 Journal of Astrophysics and Astronomy
Gaia 2
Star formation rates in the L 1482 filament of the California molecular cloud
DOI: 10.1093/pasj/psaa048 Bibcode: 2020PASJ...72...55O

Shimajiri, Yoshito; Sunada, Kazuyoshi; Dobashi, Kazuhito +7 more

We measured the trigonometric parallax of the H2O maser source associated with the L 1482 molecular filament hosting the most massive young star, LkHα 101, in the California molecular cloud. The measured parallax is 1.879 ± 0.096 mas, corresponding to the distance of 532 ± 28 pc. This parallax is consistent with that of the nearby star …

2020 Publications of the Astronomical Society of Japan
Gaia 2
The Initiation of a Solar Streamer Blowout Coronal Mass Ejection Arising from the Streamer Flank
DOI: 10.3847/2041-8213/ab9ebd Bibcode: 2020ApJ...897L..21Z

Chen, Yao; Zheng, Ruisheng; Wang, Bing

Streamer blowout (SBO) coronal mass ejections (CMEs) represent a particular class of CMEs that are characterized by a gradual swelling of the overlying streamer and a slow CME containing a flux-rope structure. SBO CMEs arising from the streamer flank fall into a special category of SBO CMEs involving three lower arches under the higher streamer ar…

2020 The Astrophysical Journal
SOHO 2
Discovery of annular X-ray emission centered on MAXI J1421-613: Dust-scattering X-rays?
DOI: 10.1093/pasj/psaa007 Bibcode: 2020PASJ...72...31N

Nobukawa, Masayoshi; Nobukawa, Kumiko K.; Yamauchi, Shigeo

We report the discovery of an annular emission of $\sim\!\! {3^{\prime }}\!-\!{9^{\prime }}$ radius around the center of a transient source, the X-ray burster MAXI J1421-613, in the Suzaku follow-up analysis. The spectrum of the annular emission shows no significant emission-line structure, and is well explained by an absorbed power-law model with…

2020 Publications of the Astronomical Society of Japan
Suzaku 2
DX Cygni: A triple system with mass transfer
DOI: 10.1016/j.newast.2019.101336 Bibcode: 2020NewA...7601336W

Wolf, M.; Mašek, M.; Kučáková, H. +2 more

A dozen of new precise times of eclipses were measured for the eclipsing binary DX Cygni as a part of our long-term observational project for studying neglected eclipsing binaries with a short orbital period. Based on a current O - C diagram, we found for the first time that its period is increasing (dP / P = 1.68 ×10-7 day/years) and t…

2020 New Astronomy
Gaia 2
A GALEX far-ultraviolet study of quasi-coeval samples of red giants
DOI: 10.1007/s10509-020-03806-5 Bibcode: 2020Ap&SS.365...95S

Smith, Graeme H.; Cochrane, Kevin M.

Samples of red giant branch (RGB) stars have been compiled from the literature for seven moving groups, and searches made for both GALEX FUV and Johnson BV photometry. It has been possible to derive a colour index

2020 Astrophysics and Space Science
Gaia 2
The Subjectivity in Identification of Martian Channel Networks and Its Implication for Citizen Science Projects
DOI: 10.1007/s11038-020-09530-y Bibcode: 2020EM&P..123...45B

Jones, M.; Bahia, R. S.

The Martian surface is incised by numerous valley networks, which indicate the planet experienced sustained widespread flowing water in the past (e.g. Carr in Water on Mars, Oxford University Press, New York, 1996; Phil Trans R Soc A 370:2193–2212, 2012. https://doi.org/10.1098/rsta.2011.0500). Examining the distribution and geometries of these va…

2020 Earth Moon and Planets
MEx 2