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Analysis of Type II and Type III Radio Bursts Associated with SEPs from Non-Interacting/Interacting Radio-Loud CMEs
DOI: 10.1007/s10511-021-09693-0 Bibcode: 2021Ap.....64..327K

Feng, Li; Prakash, O.; Shanmugaraju, A. +4 more

We analyze radio bursts observed in events with interacting/non-interacting CMEs that produced major SEPs (Ip > 10 MeV) from April 1997 to December 2014. We compare properties of meter (m), decahectometer (DH) type II and DH type III bursts, and time lags for interacting-CME-associated (IC) events and non-interacting-CME-associated (…

2021 Astrophysics
SOHO 4
Oxygen-Rich Cool Stars in the Cepheus Region. New Spectroscopic Observations of Selected Objects from the KP2001 Catalog
DOI: 10.1007/s10511-021-09681-4 Bibcode: 2021Ap.....64..203P

Gigoyan, K. S.; Kostandyan, G. R.; Petrosyan, G. V. +1 more

Spectra taken with the 2.6-m telescope at the Byurakan Astrophysical Observatory (BAO) in the λλ4000-7250Å range for eight M giants from the KP2001 catalog confirm their oxygen-rich nature. The features of these spectra are examined. Several important physical parameters from the EDR3 Gaia data base are presented. The optical variability is studie…

2021 Astrophysics
Gaia 0
Interrelationships between Halo-Type Coronal Mass Ejections and Solar Flares Based on Observations in the 23rd and 24th Cycles
DOI: 10.1007/s10511-021-09668-1 Bibcode: 2021Ap.....64...61B

Bruevich, E. A.; Burov, V. A.; Arakelov, A. S. +1 more

Solar activity of an explosive character during the 23rd and 24th cycles is analyzed. X-ray observations from the GOES-15 satellite during flares and observations during coronal mass ejections (CME) with the SOHO/LASCO coronagraph are used. The delay intervals between the onset of a flare and the onset of a Halo-type CME associated the same active…

2021 Astrophysics
SOHO 0
Orbits and Individual Masses of Some Visual Binaries
DOI: 10.1007/s10511-021-09666-3 Bibcode: 2021Ap.....64...41E

Elsanhoury, W. H.; Elkholy, E. A.; Nouh, M. I.

The orbits of visual binary systems still attract the interest of many working groups in astronomy. These orbits are the most important and reliable sources of stellar masses. In the present paper, we computed the orbits and dynamical masses of some visual binaries using an independent code. We used the Kowalsky method to compute the geometrical e…

2021 Astrophysics
Gaia 0