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Havlen-Moffat #1, el cúmulo menos pensado
Bibcode: 2020BAAA...61B.111L

Morrell, N. I.; Gamen, R. C.; Giorgi, E. E. +1 more

The cluster Havlen-Moffat # 1 (HM1), in the constellation of Scorpius, owes its name to those who discovered it in 1977. They identified, spectroscopically, two Wolf-Rayet and two Of-type stars. HM1 is located in the fourth quadrant of the Milky Way where the absorption of the interstellar medium is significant. This work presents an analysis of t…

2020 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 0
Detection of Periodicity in SiO Maser Intensity and Velocity Shift of the Symbiotic Star CH Cyg
DOI: 10.3847/2041-8213/ab9f99 Bibcode: 2020ApJ...897L..26C

Kim, Dong-Jin; Kim, Jaeheon; Cho, Se-Hyung +3 more

We performed simultaneous monitoring observations of H2O 616-523 and SiO V = 1, 2, $J=1\to $ 0, SiO V = 1, $J=2\to $ 1, $3\to 2$ maser lines toward the symbiotic star CH Cyg from 2012 December to 2019 November using the Korean very long baseline interferometry Network single-dish telescope. SiO V = 1, 2, $J=1\to 0$…

2020 The Astrophysical Journal
Gaia 0
The kinematics of OB-stars and Cepheids based on Gaia DR2 catalogue
DOI: 10.26087/INASAN.2020.5.5.012 Bibcode: 2020INASR...5..275P

Pakhomova, P. V.

The purpose of the work was to study the kinematics and refine the distance scale of young objects of the galactic disk: OB stars and high-luminosity stars of late spectral classes, as well as Cepheids. We used the observational data obtained during the Gaia mission and published in the Gaia DR2 catalog. The statistical parallax method was used to…

2020 INASAN Science Reports
Gaia 0
STARHORSE photo-astrometricdistances, extinctions, and astrophysical parameters for Gaia DR2 stars
Bibcode: 2020BAAA...61C..38A

Anders, F.; Chiappini, C.; Santiago, B. X. +2 more

By combining the precise data delivered by Gaia DR2 with the photometric catalogues of PanSTARRS-1, 2MASS, and AllWISE, we recently derived Bayesian stellar parameters, distances, and extinctions for 265 million stars. The results are available to the community through the Gaia mirror at gaia.aip.de. We remind the community to pay attention to the…

2020 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 0
Quasiperiodic Velocity Fluctuations in Eruptive Prominences Observed by AIA/SDO
DOI: 10.3847/1538-4357/ab7db6 Bibcode: 2020ApJ...893...40T

Tsvetkov, Tsvetan; Petrov, Nikola

The current study presents an investigation of the behavior of prominences during eruptions. Variations in the distribution of their velocities are detected at altitudes <0.6 R. Detailed analyses are carried out for 304 Å Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) observations. To track the behavior of promine…

2020 The Astrophysical Journal
SOHO 0
Features of Slow Sunspot Dissipation
DOI: 10.1134/S0016793219080279 Bibcode: 2020Ge&Ae..59.1055Z

Solov'ev, A. A.; Zhivanovich, I.

According to a model of sunspot dissipation through a thin boundary layer between the sunspot magnetic flux tube and the surrounding medium, the rate of decrease in the sunspot area must slow as the spot size decreases until it reaches a critical threshold at which the linear law of sunspot dissipation gives way to a nonlinear one. This theoretica…

2020 Geomagnetism and Aeronomy
SOHO 0
Agile Development of Science Operations: The Solar Orbiter Experience
Bibcode: 2020ASPC..522..335G

García-Reinaldos, María; Marcos, José; Sánchez, Luis

Cost and schedule are very rigid external constraints for the development of a Science Operations Centre (SOC), as typically the SOC is not considered a critical item for launch and cost and schedule depend on the overall project. Therefore, the greatest degree of flexibility in SOC development is the scope: while we aim to satisfy all the high le…

2020 Astronomical Data Analysis Software and Systems XXVII
SolarOrbiter 0
On the unexpected geomagnetic storm on june 8, 2019, and the heliospheric current sheet effect
DOI: 10.1016/j.pss.2020.105084 Bibcode: 2020P&SS..19305084D

Augusto, C. R. A.; Navia, C. E.; de Oliveira, M. N. +1 more

A period of minimum magnetic solar activity (such as June 2019) favors the observation of rare solar transient events, which would otherwise be lost in the magnetic vortex during a period of maximum solar activity. In this paper, we show that the most plausible explanation for the origin of an unexpected geomagnetic storm on June 8, 2019, is a sma…

2020 Planetary and Space Science
SOHO 0
Numerical simulation of ion reflection by lunar crustal magnetic fields
DOI: 10.5194/egusphere-egu2020-18137 Bibcode: 2020EGUGA..2218137D

Divin, Andrey; Deca, Jan; Lue, Charles +1 more

We investigate the dynamics of solar wind - Moon interaction by means of large-scale Particle-in-Cell (PIC) simulations in this study. Implicit moment PIC method and open boundaries are implemented in the code (iPIC3D) allowing to use large-scale domains in three dimensions. Even though the Moon has no global dipolar magnetic field, satellite magn…

2020 EGU General Assembly Conference Abstracts
Chandrayaan-1 0
Steerable High-Gain Dual-Reflector Antenna at X-Band for Solar Orbiter
DOI: 10.1109/TAP.2020.2980333 Bibcode: 2020ITAP...68.5784M

Martinez, Victor Sanchez; Jimenez, Fernando Martin; Baladron, Inaki Pinto +7 more

2020 IEEE Transactions on Antennas and Propagation
SolarOrbiter 0