Ghazaryan, S. ; Hambardzumyan, L. ; Grigoryan, A. ; Gigoyan, K. ; Michel, K.-U. ; Hambaryan, V. ; Neuhaeuser, R.
We have searched high-velocity stars (runaway, walk-away, pulsars, HMXBs and LMXBs), which could have, most probably, originated in the complex CepOB2 association, i.e. in the cores (small clusters or multiple stellar systems) of it. With the trace-back motion study of them we found at least two pairs consisting of a runaway star and pulsar, which were within stellar groups in the Cep OB2 association ∼ 1.5-5.5 Myr ago.
oai:arar.sci.am:367739
ՀՀ ԳԱԱ Հիմնարար գիտական գրադարան
Aug 1, 2024
Jan 9, 2024
19
https://arar.sci.am/publication/397479
Edition name | Date |
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Ghazaryan, S., Identification of Birth Places of High-Velocity Stars: CepOB2 Association | Aug 1, 2024 |
Hambaryan, V. Ghazaryan, S. Hambardzumyan, L. Neuhaeuser, R. Mirzoyan, A. Tsvetkova, K. P.
Gigoyan, K. K.
Gigoyan, K. S.
Kostandyan, G. R. Gigoyan, K. S.
Gigoyan, K. S. Gigoyan, K. K. Sarkissian, A. Kostandyan, G. R. Karapetyan, E. Meftah, M. Azatyan, N. Zamkotsian, F.
Karapetyan, E. L. Gigoyan, K. S. Kostandyan, G. R.