The project, funded by Science Committee of RA (ARPI program), intended to search, detection, kinematic study and identification of the birth places of the high-velocity and isolated neutron stars that encountered in the past with a stellar groups (multiple stars, stellar clusters, associations, etc.) closer than 10 pc, i.e. to test the concept: a high-velocity star and a stellar group or some of its members in the past were “in the same place at the same time”. We plan to use stars with the high-quality astrometry and radial velocities from the very recently released Gaia DR3 catalogue and empirically select high-velocity candidates. Next, by using full gravitational potential of the Galaxy to calculate the motion of a stellar groups and a candidate of high-velocity star from their current positions to the proximity epoch. For numerical integration we will utilize the fast and accurate numerical integration.
oai:arar.sci.am:361047
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Aug 1, 2024
Jul 10, 2023
43
https://arar.sci.am/publication/390317
| Edition name | Date |
|---|---|
| Hambaryan, V., Search and identification of high-velocity stars by dynamicalejection and supernovae from multiple stars | Aug 1, 2024 |
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А. М. Соболев В. С. Стрельницкий Н. Н. Чугай Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017)
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