Search Publications

New Photometric Investigation of the Solar-Type Shallow-Contact Binary HH Bootis
DOI: 10.1155/2019/5641518 Bibcode: 2019AdAst2019E...5H

He, Jia-jia; Wang, Jing-jing

Four-color charge-coupled device (CCD) light curves in $B$, $V$, $Rc$ and $Ic$ bands of the total-eclipsing binary system, V1853 Ori, are presented. By comparing our light curves with those published by previous investigators, it is detected that the O'Connell effect on the light curves is disappeared. By analyzing those multi-color light curves w…

2019 Advances in Astronomy
Gaia 0
The eastern & western elongations of Venus, 2007-'17. I. The sunlit hemisphere
Bibcode: 2019JBAA..129...73M

McKim, R. J.; Abel, P.; Leatherbarrow, W. J.

Fourteen successive morning and evening elongations of Venus from 2007-2017 are reviewed. The work of 153 observers covered the time period of ESA's Venus Express and Japan's Akatsuki missions, and wavelengths from 335-1750nm. The instantaneous rotation period of the ultraviolet markings was studied as a function of latitude, and the results compa…

2019 Journal of the British Astronomical Association
VenusExpress 0
Second Outburst of the Yellow Symbiotic Star LT Delphini
DOI: 10.1134/S1063773719050025 Bibcode: 2019AstL...45..361I

Arkhipova, V. P.; Ikonnikova, N. P.; Komissarova, G. V.

We present the results of our photoelectric UBV observations of the yellow symbiotic star LT Del over 2010-2018. The binary system LT Del, which consists of a bright K giant and a compact hot star with a temperature of 100 000 K, has an orbital period of 476 days. In 2017 the variable experienced a second low-amplitude (Δ V 07) outbu…

2019 Astronomy Letters
Gaia 0
Ground-based Paα narrow-band imaging of local luminous infrared galaxies. II. Bulge structure and star formation activity
DOI: 10.1093/pasj/psz042 Bibcode: 2019PASJ...71...64T

Komugi, Shinya; Takahashi, Hidenori; Doi, Mamoru +8 more

We present properties of two types of bulges (classical and pseudobulges) in 20 luminous infrared galaxies observed in the near infrared of the H, Ks, and 1.91µm narrow-band targeting of the hydrogen Paα emission line by the University of Tokyo Atacama Observatory 1 m telescope. To classify the two types of bulges, we first perfor…

2019 Publications of the Astronomical Society of Japan
eHST 0
Probabilistic galeeactic dynamics - I. The Sun and GJ 710 with Monte Carlo, linearized, and unscented treatments
DOI: 10.1093/mnras/sty3333 Bibcode: 2019MNRAS.483.3971F

Jones, H. R. A.; Feng, F.

Deterministic galactic dynamics is impossible due to a lack of precise knowledge of the initial conditions and galactic potential. Instead of treating stellar orbits deterministically, we integrate not only the mean but also the covariance of a stellar orbit in the Galaxy. As a test case, we study the probabilistic dynamics of the Sun and the star…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 0
The intermediate age population of the Galactic halo
DOI: 10.1007/s10509-019-3533-0 Bibcode: 2019Ap&SS.364...42M

Mould, Jeremy

We have learned recently that the inner halo of the Milky Way contains a kinematically coherent component (Gaia-Enceladus) from a significant merger 10 Gyrs ago. By contrast the inner (defined to exclude the Magellanic Stream) halo contains no similar intruder stellar population of billion year age. The tracer we use to set the corresponding upper…

2019 Astrophysics and Space Science
Gaia 0
Central Wavelengths and Profile Shapes of Diffuse Interstellar Bands versus Physical Parameters of Intervening Clouds
DOI: 10.32023/0001-5237/69.4.5 Bibcode: 2019AcA....69..369K

Krełowski, J.; Galazutdinov, G. A.; Marić, T. +2 more

We investigate whether there are variations of the central wavelengths or the profile shapes of diffuse interstellar bands and whether these variations are caused by different physical parameters of translucent clouds. For this purpose we used spectra of two stars seen through two different single clouds: HD 34078 (AE Aur) and HD 73882. The wavele…

2019 Acta Astronomica
Gaia 0
Corrigendum to "Neptune's carbon monoxide profile and phosphine upper limits from Herschel/SPIRE" (Icarus, vol 319, p86-98, 2019)
DOI: 10.1016/j.icarus.2018.11.033 Bibcode: 2019Icar..322..261T

Irwin, P. G. J.; Teanby, N. A.; Moses, J. I.

The authors would like to publish the below information which was incorrectly published in its original version.

2019 Icarus
Herschel 0
Black coatings for combined stray light and thermal passive management for the challenging environmental conditions of Solar Orbiter
DOI: 10.1117/12.2536097 Bibcode: 2019SPIE11180E..4YM

Castronuovo, Marco; Schillaci, Tiziano; Montemurro, Luca +4 more

In the context of ESA's Cosmic Vision 2015-2025 scientific program, Solar Orbiter (SolO) represents the first M-class mission, currently under implementation for a launch planned in October 2018.
One of the SolO solar remote-sensing instruments is the Multi Element Telescope for Imaging and Spectroscopy (METIS), under development by an Italia…

2019 International Conference on Space Optics — ICSO 2018
SolarOrbiter 0
Metis/Solar Orbiter polarimetric visible light channel calibration
DOI: 10.1117/12.2536039 Bibcode: 2019SPIE11180E..3CC

Romoli, M.; Andretta, V.; Uslenghi, M. +16 more

Metis is the solar coronagraph of the ESA mission Solar Orbiter. For the first time, Metis will acquire simultaneous images of the solar corona in linearly polarized, broadband visible light (580-640 nm) and in the narrow-band HI Ly-α line (121.6 nm). The visible light path includes a polarimeter, designed to observe and analyse the K-corona linea…

2019 International Conference on Space Optics — ICSO 2018
SolarOrbiter 0