In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 47, no. 2
L. Chmyreva - G. Beskin - S. Karpov
Detaily:
Rok, strany: 2017, 137 - 142
Kľúčové slová:
radio pulsars, black holes, kinematics
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2017/Vol_47/No_2/pp137-142_abstract.html
O článku:
We performed a search for isolated stellar-mass black hole candidates
based on the fact that more than 50% of radio pulsars have originated in
binary systems, now disrupted, where the other component could have evolved
into a black hole prior to the second supernova event in the system which
caused its disruption. To this end, several relatively young isolated
pulsars with known parallaxes fitting the selection criteria were traced
back to their presumed birth locations. These areas were then analyzed for
possible black hole candidates based on the astrometric, photometric, and
spectral data available. We present the results for the first 4 pulsars in
our sample, J0139+5814, J0922+0638, J0358+5413, and J1395+1616. Several
possible candidates were selected for further analysis.
Ako citovať:
ISO 690:
Chmyreva, L., Beskin, G., Karpov, S. 2017. Searching for isolated stellar-mass black hole candidates by analyzing the kinematics of their former companions in disrupted binary systems. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 47, no.2, pp. 137-142. 1335-1842.
APA:
Chmyreva, L., Beskin, G., Karpov, S. (2017). Searching for isolated stellar-mass black hole candidates by analyzing the kinematics of their former companions in disrupted binary systems. Contributions of the Astronomical Observatory Skalnaté Pleso, 47(2), 137-142. 1335-1842.