Abstract
We present the results of our CCD photometric and moderate-dispersion spectroscopic observations of the binary system V4641 Sgr, which contains a black hole of mass ≈9.5M ⊙ and a normal B9III star. The photometric light curve reveals an ellipticity effect with very high amplitudes in V and R, 0.40m and 0.37m, and the color curve shows that the surface temperature is nonuniform. All this testifies to tidal distortion of the normal star's surface due to the massive companion and to a high inclination of the orbit to the line of sight. In June and July 2002, during quiescence, we obtained data during three flares with amplitudes up to 0.26m. In particular, spectroscopic observations were acquired near the time of the black hole's inferior conjunction. One hour before conjunction, a depression by EW=0.5 Å was observed in the red wing of the Hα absorption line, interpreted as absorption by gas flowing in the direction from the observer toward the normal star. This flow is apparently associated with a rarefied gas disk around the black hole, and the conjunction grazes the stellar surface if the orbital inclination is close to 70.7°. The maximum velocity along a circular Keplerian orbit is 650 km/s at a distance of R=0.15–0.20a from the black hole (where a is the component separation). Thus, we find the mass of the black hole to be M BH =7.1–9.5M ⊙, confirming the model of Orosz et al. (2001).
Similar content being viewed by others
References
V. P. Goranskij, Astron. Tsirk., No. 1024, 3 (1978).
V. P. Goranskij, Inform. Bull. Var. Stars, No. 3464 (1990).
M. L. Hazen, D. Hoffleit, B. L. Welther, and D. B. Williams, AAVSO J. 28, 99 (2000).
J. Orosz, Inform. Bull. Var. Stars, No. 4921 (2000).
J. in't Zand, J. Heize, A. Bazzano, et al., IAU Circ. No. 7119 (1999).
C. B. Markwardt, J. H. Swank, and F. E. Marshall, IAU Circ. No. 7120 (1999).
T. Kato, M. Uemura, R. Stubbings, et al., Inform. Bull. Var. Stars, No. 4777 (1999).
M. Uemura, T. Kato, T. Watanabe, et al., Publ. Astron. Soc. Jpn. 54, 95 (2002).
R. Stubbings, IAU Circ. No. 7253 (1999).
K. Ayani, T. C. Peiris, and A. C. Clarke, IAU Circ. No. 7254 (1999).
S. G. Djorgovski, R. R. Gal, A. Mahabal, et al., ATEL No. 44 (1999).
P. A. Charles, T. Shahbaz, and T. Geballe, IAU Circ. No. 7267 (1999).
S. Chaty, I. F. Mirabel, J. Marti, and L. F. Rodriguez, Astrophys. Space Sci. 276, 153 (2001), astro-ph/0102105.
R. M. Hjellming, M. P. Rupen, R. W. Hunstead, et al., Astrophys. J. 544, 977 (2000).
D. A. Smith, A. M. Levine, and E. H. Morgan, IAU Circ. No. 7253 (1999).
R. Wijnands and M. van der Klis, Astrophys. J. 528, L93 (2000).
J. J. M. in't Zand, E. Kuulkers, A. Bazzano, et al., Astron. Astrophys. 357, 520 (2000).
M. G. Revnivtsev and R. A. Syunyaev, Pis'ma Astron. Zh. 28, 83 (2002) [Astron. Lett. 28, 69 (2002)].
M. Revnivtsev, R. Sunyaev, M. Gilfanov, and E. Churazov, Astron. Astrophys. 385, 904 (2002).
M. Revnivtsev, M. Gilfanov, E. Churazov, and R. Sunyaev, Astron. Astrophys. 391, 1013 (2002).
M. Uemura, T. Kato, R. Ishioka, et al., Publ. Astron. Soc. Jpn. (in press, 2002); astro-ph/0208146.
M. Rupen, V. Dhavan, and A. Mioduszewski, IAU Circ. No. 7928 (2002).
D. Campbell-Wilson and R. W. Hunstead, IAU Circ. No. 7908 (2002).
C. B. Markwardt and J. H. Swank, IAU Circ. No. 7906 (2002).
J. A. Tomsick, M. P. Rupen, S. Corbel, et al., ATEL No. 105 (2002).
R. M. Hjellming, ATEL No. 62 (2000).
J. Orosz, E. Kuulkers, M. van der Klis, et al., Astrophys. J. 555, 489 (2001).
V. P. Goranskij, E. A. Barsukova, A. H. Burenkov, and D. N. Monin, in New Views on Microquasars, Ed. by Ph. Durouchoux, V. Fuchs, and J. Rodrigues (Center for Space Physics, Kolkata, 2002, in press); astro-ph/0209592.
A. Henden, vsnet-campaign-v4641sgr. No. 133 (VSNET, 2002).
V. P. Goranskij, Inform. Bull. Variable Stars, No. 5068 (2001).
J. Marti, R. Zamanov, J. M. Paredes, and M. Ribo, Inform. Bull. Var. Stars, No. 5036 (2001).
E. A. Karitskaya, Candidate's Dissertation in Mathematical Physics (Moscow, Sternberg Astron. Inst., 1982).
A. V. Goncharskij, S. Yu. Romanov, and A. M. Cherepachshuk, Astrophysic Finite-Parametric Inverse Problems (Mos. Gos. Univ., Moscow, 1991), p. 77.
E. A. Karitskaya, I. B. Voloshina, V. P. Goranskij, et al., Astron. Zh. 78, 408 (2001) [Astron. Rep. 45, 350 (2001)].
V. P. Goranskij and V. M. Lyuty, Astron. Zh. 65, 381 (1988) [Sov. Astron. 32, 193 (1988)].
M. Rupen, vsnet-campaign-v4641sgr No. 104 (VSNET, 2002).
Author information
Authors and Affiliations
Additional information
__________
Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 80, No. 9, 2003, pp. 805–815.
Original Russian Text Copyright © 2003 by Goranskij, Barsukova, Burenkov.
Rights and permissions
About this article
Cite this article
Goranskij, V.P., Barsukova, E.A. & Burenkov, A.N. Photometry and spectroscopy of the system V4641 sagittarii in quiescence. Astron. Rep. 47, 740–749 (2003). https://doi.org/10.1134/1.1611215
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1134/1.1611215