Search Publications

Quantifying torque from the Milky Way bar using Gaia DR2
DOI: 10.1093/mnras/staa929 Bibcode: 2020MNRAS.494.3358K

Kipper, Rain; Tenjes, Peeter; Tuvikene, Taavi +2 more

We determine the mass of the Milky Way bar and the torque it causes, using Gaia DR2, by applying the orbital arc method. Based on this, we have found that the gravitational acceleration is not directed towards the centre of our Galaxy but a few degrees away from it. We propose that the tangential acceleration component is caused by the bar of the …

2020 Monthly Notices of the Royal Astronomical Society
Gaia 7
A Catalog of Periodic Variables in Open Clusters M35 and NGC 2158
DOI: 10.3847/1538-4365/ab5fcf Bibcode: 2020ApJS..246...15S

Bouma, L. G.; Bhatti, W.; Bakos, G. Á. +3 more

We present a catalog of 1143 periodic variables, compiled from our image-subtracted photometric analysis of the K2 Campaign-0 super stamp. This super stamp is centered on the open clusters M35 and NGC 2158. Approximately 46% of our periodic variables were previously unreported. Of the catalog variables, we find that 331 are members of M35 and 56 a…

2020 The Astrophysical Journal Supplement Series
Gaia 7
SOIR/VEx observations of water vapor at the terminator in the Venus mesosphere
DOI: 10.1016/j.icarus.2020.113819 Bibcode: 2020Icar..34613819C

Vandaele, A. C.; Trompet, L.; Robert, S. +4 more

The Solar Occultation in the InfraRed (SOIR) instrument onboard Venus Express sounded the Venus mesosphere and lower thermosphere using solar occultation geometry between April 2006 and December 2014. The observations were all taken at the terminator. This paper reports on the water vapor vertical distribution above the clouds and geo-temporal var…

2020 Icarus
VenusExpress 7
HST/COS Spectra of the Wind Lines of VFTS 102 and 285
DOI: 10.3847/1538-4357/ab5a82 Bibcode: 2020ApJ...888...82S

Gies, Douglas R.; Lester, Kathryn V.; Wang, Luqian +5 more

Rapid rotation in massive stars imposes a latitudinal variation in the mass loss from radiatively driven winds that can lead to enhanced mass loss at the poles (with little angular momentum loss) and/or equator (with maximal angular momentum loss). Here we present an examination of the stellar wind lines of the two O-type stars with the fastest kn…

2020 The Astrophysical Journal
IUE eHST 7
Modeling the IRIS Lines During a Flare. I. The Blue-wing Enhancement in the Mg II k Line
DOI: 10.3847/1538-4357/ab6d05 Bibcode: 2020ApJ...890..115H

Ding, M. D.; Li, Ying; Hong, Jie +1 more

The Interface Region Imaging Spectrograph (IRIS) Mg II k line serves as a very good tool to diagnose the heating processes in solar flares. Recent studies have shown that apart from the usual red asymmetries that are interpreted as the result of condensation downflows, this line could also show a blue-wing enhancement. To investigate how such a bl…

2020 The Astrophysical Journal
IRIS 7
A model of the 3-µm hydration band with Exponentially Modified Gaussian (EMG) profiles: Application to hydrated chondrites and asteroids
DOI: 10.1016/j.icarus.2020.113686 Bibcode: 2020Icar..34313686P

Schmitt, B.; Beck, P.; Potin, S. +2 more

We present here a new method to model the shape of the 3-µm absorption band in the reflectance spectra of meteorites and small bodies. The band is decomposed into several OH/H2O components using Exponentially Modified Gaussian (EMG) profiles, as well as possible organic components using Gaussian profiles when present. We compare t…

2020 Icarus
AKARI 7
A Geoeffective CME Caused by the Eruption of a Quiescent Prominence on 29 September 2013
DOI: 10.1007/s11207-020-01619-x Bibcode: 2020SoPh..295...55G

Grechnev, V. V.; Kuzmenko, I. V.

The eruption of a large prominence that occurred away of active regions in the SOL2013-09-29 event produced a fast coronal mass ejection (CME) and a shock wave. The event caused considerable geospace disturbances, including a proton enhancement that have been addressed in previous studies. Continuing with the analysis of this event, we focus on th…

2020 Solar Physics
SOHO 7
A broadband X-ray view of the NLSy1 1E 0754.6+3928
DOI: 10.1051/0004-6361/201936701 Bibcode: 2020A&A...635A..18M

Bianchi, S.; Petrucci, P. -O.; Miniutti, G. +8 more

Context. The soft X-ray band of many active galactic nuclei (AGNs) is affected by obscuration due to partially ionised matter crossing our line of sight. In this context, two past XMM-Newton observations that were six months apart and a simultaneous NuSTAR-Swift exposure of the Narrow Line Seyfert 1 galaxy 1E 0754.6+3928, which was approximately e…

2020 Astronomy and Astrophysics
XMM-Newton 7
Determination of the Configurations of Boundaries in Space
DOI: 10.1029/2020JA028163 Bibcode: 2020JGRA..12528163S

Russell, C. T.; Dunlop, M.; Rong, Zhaojin +5 more

This research aims to determine the geometrical configurations of boundary surfaces in the space environment, based on multiple spacecraft measurements. To achieve this, the Normal Field Analysis (NFA) method is presented here. With multipoint observations, the three-dimensional gradient of the normal of boundary layers can be obtained, and the pr…

2020 Journal of Geophysical Research (Space Physics)
Cluster 7
Gaia DR2 data and the evolutionary status of eight high-velocity hot post-AGB candidates
DOI: 10.1093/pasj/psaa097 Bibcode: 2020PASJ...72...99P

Matsuno, Tadafumi; Aoki, Wako; Parthasarathy, Mudumba

From Gaia DR2 data of eight high-velocity hot post-AGB candidates, LS 3593, LSE 148, LS 5107, HD 172324, HD 214539, LS IV -12 111, LS III +52 24, and LS 3099, we found that six of them have accurate parallaxes which made it possible to derive their distances, absolute visual magnitudes (MV) and luminosity (log L/L). All the …

2020 Publications of the Astronomical Society of Japan
Gaia 7