Search Publications

Investigation of faint galactic carbon stars from the First Byurakan Spectral Sky Survey. IV. GAIA DR2 data
DOI: 10.52526/25792776-2020.67.2-206 Bibcode: 2020CoBAO..67..206K

Kostandyan, G. R.

The second Gaia data release (Gaia DR2) data are used to analyze and estimate some important parameters for 127 carbon (C) type stars (56 are late N - type Asymptotic Giant Branch (AGB) C stars, 71 are early type CH giants) detected on the First Byurakan Spectral Sky Survey (FBS) low-resolution (lr) spectral plates. Gaia DR2 G broad band magnitude…

2020 Communications of the Byurakan Astrophysical Observatory
Gaia 1
Binary star detection in the open cluster King 1 field
DOI: 10.1088/1674-4527/20/3/43 Bibcode: 2020RAA....20...43S

Saleh, Parvej Reja; Hazarika, Debasish; Dar, Ajaz Ahmad +2 more

A rarely studied open cluster, King 1 is observed using the 1.3-m telescope equipped with a 2k × 4k CCD at Vainu Bappu Observatory, India. We analyze the photometric data obtained from CCD observations in both B and V bands. Out of 132 detected stars in the open cluster King 1 field, we have identified four stellar variables, and two among them ar…

2020 Research in Astronomy and Astrophysics
Gaia 1
On the Formation of Lyman β and the O I 1027 and 1028 Å Spectral Lines
DOI: 10.3847/1538-4357/aba95c Bibcode: 2020ApJ...900...34H

Carlsson, Mats; Shimizu, Toshifumi; Hasegawa, Takahiro +1 more

We study the potential of Lyman β and the O I 1027 and 1028 Å spectral lines to help in understanding the properties of the chromosphere and transition region (TR). The oxygen transitions are located in the wing of Lyman β, which is a candidate spectral line for the solar missions Solar Orbiter/Spectral Imaging of the Coronal Environment and Solar…

2020 The Astrophysical Journal
SOHO 1
Simultaneous Polar and Cluster Observations in the Northern and Southern Middle-Altitude Polar Cusps Around Equinox
DOI: 10.1029/2020JA028346 Bibcode: 2020JGRA..12528346P

Berchem, J.; Escoubet, C. P.; Pitout, F. +3 more

We present an event of simultaneous observations of the northern and southern middle-altitude polar cusps by the Polar spacecraft and Cluster fleet that occurred on 23 September 2004. We examine the possible asymmetries in the fields and plasma parameters, although the proximity of the equinox should limit these asymmetries. Ion sensors reveal two…

2020 Journal of Geophysical Research (Space Physics)
Cluster 1
Development of a simulator of the SIMBIOSYS suite onboard the BepiColombo mission
DOI: 10.1093/mnras/stz3060 Bibcode: 2020MNRAS.491.1673S

Cremonese, G.; Da Deppo, V.; Capaccioni, F. +11 more

BepiColombo is the fifth cornerstone mission of the European Space Agency (ESA) dedicated to study the Mercury planet. The BepiColombo spacecraft comprises two science modules: the Mercury Planetary Orbiter (MPO) realized by ESA and the Mercury Magnetospheric Orbiter provided by the Japan Aerospace Exploration Agency. The MPO is composed by 11 ins…

2020 Monthly Notices of the Royal Astronomical Society
BepiColombo 1
Electron Density Reconstruction of Solar Coronal Mass Ejections Based on a Genetic Algorithm: Method and Application
DOI: 10.3847/1538-4357/ab963a Bibcode: 2020ApJ...896..155D

Inhester, Bernd; Wang, Huaning; Dai, Xinghua

We present a new method to reconstruct the three-dimensional electron density of coronal mass ejections (CMEs) based on a genetic algorithm, namely the genetic reconstruction method (GRM). GRM is first applied to model CMEs with different orientations and shapes. A set of analytic model CMEs from Gibson and Low is employed to produce synthetic CME…

2020 The Astrophysical Journal
SOHO 1
The importance of studying active giant stars in eclipsing binaries - and the role of citizen scientists in finding them
DOI: 10.31577/caosp.2020.50.2.390 Bibcode: 2020CoSka..50..390O

Derekas, A.; Vanderburg, A.; Rappaport, S. +2 more

Red giant stars with deep convection zones and rapid rotation maintain a strong surface magnetic field which may alter their observable astrophysical parameters. The resulting lower surface temperature due to spots makes the inferred masses and ages from evolutionary tracks uncertain. Eclipsing binaries having an active giant component can help in…

2020 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 1
Ammonia in circumstellar environment of V Cyg
DOI: 10.17721/2227-1481.10.7-11 Bibcode: 2020AASP...10....7E

Szczerba, R.; Etmański, B.; Schmidt, M. R.

The HIFI instrument on board of the Herschel Space Observatory (HSO) has been very successful in detecting molecular lines from the circumstellar envelopes around evolved stars, like massive red supergiants, Asymptotic Giant Branch (AGB) and post-AGB stars, as well as the planetary nebulae. Among others, ammonia have been found in the circumstella…

2020 Advances in Astronomy and Space Physics
Herschel ISO 1
Multifrequency study of HH 137 and HH 138: discovering new knots and molecular outflows with Gemini and APEX
DOI: 10.1093/mnras/staa1863 Bibcode: 2020MNRAS.496.4239F

Rubio, Mónica; Saldaño, Hugo P.; Gómez, Mercedes +3 more

We present a multiwavelength study of two Herbig-Haro (HH) objects (137 and 138) that may be associated. We use Gemini H2 (2.12 µm) and K (2.2 µm) images, as well as Atacama Pathfinder EXperiment molecular line observations and Spitzer image archives. Several H2 knots, linked to the optical chain of knots of HH 13…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 1
Comparison of Magnetic and Plasma Overshoots of Interplanetary Shocks
DOI: 10.1134/S0010952520060015 Bibcode: 2020CosRe..58..450B

Yermolaev, Yu. I.; Eselevich, V. G.; Zastenker, G. N. +2 more

The structure of interplanetary shock fronts was studied based on the data from the BMSW plasma spectrometer, installed on the SPEKTR-R spacecraft, supplemented by magnetic field measurements on the WIND spacecraft. Special attention was paid to periodic growths (overshoots) in the value of the ion flux or magnetic field relative to their mean val…

2020 Cosmic Research
Cluster 1