We searched for the high-velocity and isolated neutron stars that encountered in the past with a stellar cluster/association closer than 20 pc. We took about 830000 stars with the high-quality astrometry and radial velocities from the Gaia DR2 catalogue and empirically selected about 560 high-velocity stars. We used a full gravitational potential of the Galaxy to calculate the motion of a stellar cluster/association and a candidate of high-velocity star from their current positions to the proximity epoch. For these calculations we used a numerical integration in rectangular, Galactocentric coordinates. We used a covariance matrices of the astrometric data for each star to estimate the accuracy of the obtained proximity distance and epoch. For this aim we used a Monte Carlo method, replaced each star with 10 000 of its simulations and studied the distribution of their individual close passages near a stellar cluster/association. In addition, we investigated a neutron star/runaway star pairs very likely both ejected from binary system during supernova event.
oai:arar.sci.am:379964
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Dec 6, 2024
Dec 6, 2024
4
https://arar.sci.am/publication/321023
Հրատարակության անուն | Ամսաթիվ |
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Hambaryan, V., Identifying birth places of high-velocity stars | Dec 6, 2024 |
Nikoghosyan, E. H. Harutyunian, H. A. Azatyan, N. M. Grigoryan, A. M.
Andronov, Ivan L. Andrych, Kateryna D. Chinarova, Lidia L. Tvardovskyi, Dmytro E.
Hambaryan, V. Neuhaeuser, R.
R. Neuhauser V. Hambaryan Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)
L. V. Mirzoyan V. V. Hambaryan A. L. Mirzoyan Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)
K. S. Gigoyan V. V. Hambaryan H. V. Abrahamyan Գլխավոր խմբ․՝ Վ․ Հ․ Համբարձումյան (1965-1987) Լ․ Վ․ Միրզոյան (1988-1999) Դ․ Մ․ Սեդրակյան (2000-2017) Ա․ Գ․ Նիկողոսյան (2018-)