We consider the low-mass flare stars which form the bulk of the population in the galactic bulge as a source of the positrons needed to form the observed narrow annihilation line from the galactic bulge. Estimates based on the observed flares in low-mass stars, together with observations of the annihilation line in solar flares, show that the rate of production of positrons in flares in the stars in the bulge may be sufficient to explain the formation of the narrow stationary annihilation line observed from the region of the galactic bulge.
Similar content being viewed by others
References
M. Leventhal, C. J. MacCallum, and P. D. Stang, Astrophys. J. 225, L11 (1978).
W. R. Purcell, D. A. Grabelsky, M. P. Ulmer, et al., Astrophys. J. 413, L85 (1993).
W. R. Purcell, L.-X. Cheng, D. D. Dixon, et al., Astrophys. J. 491, 725 (1997).
P. Jean, J. Knodlseder, V. Lonjou, et al., Astron. Astrophys. 407, L55 (2003).
E. Churazov, S. Sazonov, S. Tsygankov, et al., Mon. Not. Roy. Astron. Soc. 411, 1727 (2011).
T. Siegert, R. Diehl, G. Khachatryan, et al., Astron. Astrophys. 586, A84 (2016).
N. Prantzos, Astron. Astrophys. 449, 869 (2006).
A. Alexis, P. Jean, P. Martin, and K. Ferrière, Astron. Astrophys. 564, A108 (2014).
T. Siegert, R. Diehl, J. Greiner, et al., Nature 531, 341 (2016).
E. Parizot, M. Cassê, R. Lehoucq, and J. Paul, Astron. Astrophys. 432, 889 (2005).
K. S. Cheng, D. O. Chernyshov, and V. A. Dogiel, Astrophys. J. 645, 1138 (2006).
T. A. Totani, PASJ 58, 965 (2006).
M. Pshirkov, Physical Review D 94, 103002 (2016).
Y. Ascasibar, P. Jean, C. Boehm, and J. Knödlseder, Mon. Not. Roy. Astron. Soc. 368, 1695 (2006).
J.-R. Cudell, M. Yu. Khlopov, and Q. Wallemacq, eprint arXiv:1401.5228 (2014).
G. H. Share, R. J. Murphy, J. G. Skibo, et al., Astrophys. J. 595, L85 (2003).
R. J. Murphy, G. H. Share, J. G. Skibo, and B. Kozlovsky, Astrophys. J. Suppl. 161, 495 (2005).
G. D. Fleishman, A. T. Altyntsev, and N. S. Meshalkina, Publ. Astron. Soc. of Japan 65, S7 (2013).
V. B. Berestetskii, E. M. Lifshitz, and L. P. Pitaevskii, Relativistic Quantum Theory Vol. 4, Pergamon Press (1971).
P. B. Esposito, P. Edenhofer, and E. Lueneburg, Journal of Geophysical Research 85, 3414 (1980).
C. J. Schrijver, J. Beer, U. Baltensperger, et al., Journal of Geophysical Research: Space Physics 117, A08103 (2012).
M. Kitze, R. Neuhäuser, V. Hambaryan, and C. Ginski, Mon. Not. Roy. Astron. Soc. 442, 3769 (2014).
S. Candelaresi, A. Hillier, H. Maehara, et al., Astrophys. J. 792, 67 (2014).
Chi-Ju Wu, Wing-Huen Ip, and Li-Ching Huang, Astrophys. J. 798, 92 (2015).
E. Valenti, M. Zoccali, O. A. Gonzalez, et al., Astron. Astrophys. 587, L6 (2015).
G. van de Ven, R. C. E. van den Bosch, E. K. Verolme, and P. T. de Zeeuw, Astron. Astrophys. 445, 513 (2006).
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated from Astrofizika, Vol. 60, No. 2, pp. 243-248 (May 2017).
Rights and permissions
About this article
Cite this article
Bisnovatyi-Kogan, G.S., Pozanenko, A.S. Can Flare Stars Explain the Annihilation Line from the Galactic Bulge?. Astrophysics 60, 223–227 (2017). https://doi.org/10.1007/s10511-017-9477-6
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10511-017-9477-6