Optical investigations of X-ray binary systems

A. M. Cherepaschuk

Učënye zapiski Kazanskogo universiteta. Seriâ Fiziko-matematičeskie nauki, Uchenye Zapiski Kazanskogo Universiteta. Seriya Fiziko-Matematicheskie Nauki, Tome 153 (2011) no. 2, pp. 20-32

Résumé

Methods and results of optical investigations of X-ray binary systems are described. Recent data on the masses of stellar-mass black holes are summarized. Some new results of demographic investigations of black holes are presented. These results allow us to study birth and evolution of black holes of different masses and reveal a connection between black holes and other objects in the Universe: stars, galaxies, etc.

Détail

Keywords: black holes, X-ray binary systems, black holes demography.

Bibliographie

[1] Cherepaschuk A. M., “Poiski chernykh dyr”, Usp. fiz. nauk, 173:4 (2003), 345–384 | DOI

[2] Zeldovich Ya. B., Novikov I. D., Teoriya tyagoteniya i evolyutsiya zvezd, Nauka, M., 1971, 484 pp. | Zbl

[3] Novikov I. D., Frolov V. P., Fizika chernykh dyr, Nauka, M., 1986, 328 pp.

[4] Thorne K. S., Price R. H., Macdonald D. A., Black Holes: the Membrane Paradigm, Yale Univ. Press, New Haven, 1986, 416 pp. | MR

[5] Logunov A. A., Teoriya gravitatsionnogo polya, Nauka, M., 2001, 240 pp. | MR

[6] Zeldovich Ya. B., “Sudba zvezdy i vydelenie gravitatsionnoi energii”, Dokl. AN SSSR, 155:1 (1964), 67–70

[7] Salpeter E. E., “Accretion of Interstellar Matter by Massive Objects”, Astrophys. J., 140 (1964), 796–800 | DOI

[8] Shakura N. I., Sunyaev R. A., “Black holes in binary systems. Observational appearance”, Astron. Astrophys., 24 (1973), 337–355

[9] Pringle J. E., Rees M. J., “Accretion Disc Models for Compact X-Ray Sources”, Astron. Astrophys., 21 (1972), 1–9

[10] Novikov I. D., Thorne K. S., “Astrophysics of Black Holes”, Black Holes, eds. C. DeWitt, B. DeWitt, Gordon and Breach, N.Y., 1973, 343–450

[11] Giacconi R., Gursky H., Kellog E., Schreier E., Tananbaum H., “Discovery of Periodic X-Ray Pulsations in Centaurus X-3 from UHURU”, Astrophys. J., 167 (1971), L67–L73 | DOI

[12] Kurochkin N. E., “Fotograficheskie nablyudeniya HZ Her=Her X-1”, Peremennye zvezdy, 18 (1972), 425–434

[13] Cherepashchuk A. M., Efremov Yu. N., Kurochkin N. E., Shakura N. I., Sunyaev R. A., “On the Nature of the Optical Variations of HZ Her=Her X-1”, Inform. Bull. Variable Stars, 720 (1972), 1

[14] Lyutyi V. M., Syunyaev R. A., Cherepaschuk A. M., “Priroda opticheskoi peremennosti HZ Herculis (Her X-l) i $\mathrm{BD}+34^\circ3815$ (Cyg X-l)”, Astron. zhurn., 50 (1973), 3–11

[15] Cherepashchuk A. M., “SS 433 as an eclipsing binary”, Mon. Not. R. Astron. Soc., 194 (1981), 761–769 | DOI

[16] Cherepashchuk A. M., Katysheva N. A., Khruzina T. S., Shugarov S. Yu., Highly Evolved Close Binary Stars, Catalog, Gordon and Breach Publ., Amsterdam, 1996, 368 pp.

[17] Antokhina E. A., Cherepaschuk A. M., “Sintez krivykh luchevykh skorostei tesnykh dvoinykh sistem”, Astron. zhurn., 71 (1994), 420–430

[18] Antokhina E. A., Cherepaschuk A. M., Shimanskii V. V., “Krivye luchevykh skorostei i teoreticheskie profili spektralnykh linii zvezd v malomassivnykh tesnykh rentgenovskikh dvoinykh sistemakh”, Astron. zhurn., 82 (2005), 131–148

[19] Cherepashchuk A. M., “Synthesis of Line Profiles and Radial Velocity Curves for X-Ray Binary Systems”, Astrophys. Space Sci., 304 (2006), 263–266 | DOI

[20] Sakhibullin N. A., Metody modelirovaniya v astrofizike, v. I, Zvezdnye atmosfery, Fen, Kazan, 1997, 328 pp.

[21] Goncharskii A. V., Romanov S. Yu., Cherepaschuk A. M., Konechnoparametricheskie obratnye zadachi astrofiziki, Izd-vo Mosk. un-ta, M., 1991, 192 pp.

[22] Abubekerov M. K., Antokhina E. A., Cherepaschuk A. M., “Massy rentgenovskikh pulsarov v dvoinykh sistemakh s OV-sverkhgigantami”, Astron. zhurn., 81 (2004), 108–123

[23] Abubekerov M. K., Antokhina E. A., Cherepaschuk A. M., “Otsenka massy chernoi dyry i nakloneniya orbity po krivoi luchevykh skorostei v rentgenovskoi dvoinoi sisteme Cyg X-1”, Astron. zhurn., 81 (2004), 606–619

[24] Abubekerov M. K., Antokhina E. A., Cherepaschuk A. M., Shimanskii V. V., “Massa kompaktnogo ob'ekta v malomassivnoi rentgenovskoi dvoinoi sisteme 2S 0921-630”, Astron. zhurn., 83 (2006), 602–619

[25] Martynov D. Ya., “Tesnye dvoinye zvezdy i ikh znachenie dlya teorii zvezdnoi evolyutsii”, Usp. fiz. nauk, 108:4 (1972), 701–732 | DOI

[26] Cherepaschuk A. M., “Zvezdy Volfa–Raie i relyativistskie ob'ekty: razlichie raspredelenii mass v tesnykh dvoinykh sistemakh”, Astron. zhurn., 78:2 (2001), 145–164

[27] Cherepaschuk A. M., “Zvezdy Volfa–Raie i relyativistskie ob'ekty”, Usp. fiz. nauk, 172:8 (2002), 959–963 | DOI

[28] Postnov K. A., Cherepaschuk A. M., “Massy zvezdnykh chernykh dyr i vozmozhnosti proverki teorii gravitatsii”, Astron. zhurn., 80:12 (2003), 1075–1085

[29] Randall L., Sundrom R., “An Alternative to Compactification”, Phys. Rev. Lett., 83 (1999), 4690–4693 | DOI | MR | Zbl

[30] Hawking S. W., “Black hole explosions?”, Nature, 248 (1974), 30–31 | DOI

[31] Long J. C., “Tests actuels de la loi en inverse carre de la gravite”, Comptes Rendus Physique, 4 (2003), 337–346 | DOI

[32] Johannsen T., Psaltis D., McClintock J. E., “Constraints on the Size of Extra Dimensions from the Orbital Evolution of Black-Hole X-Ray Binaries”, Astrophys. J., 691 (2009), 997–1004 | DOI

[33] Postnov K. A., Prokhorov M. E., “Svyaz nablyudaemogo raspredeleniya mass kompaktnykh zvezd s mekhanizmom vspyshek sverkhnovykh”, Astron. zhurn., 78:11 (2001), 1025–1033

[34] Fryer C. L., Kalogera V., “Theoretical Black Hole Mass Distributions”, Astrophys. J., 554 (2001), 548–560 | DOI

[35] Tutukov A. V., Cherepaschuk A. M., “Massivnye tesnye dvoinye zvezdy i gamma-barstery”, Astron. zhurn., 81 (2004), 43–49