PACS numbers

95.30.−k Fundamental aspects of astrophysics
  1. Yu.A. Shchekinov, V.N. Lukash et alInterstellar and intergalactic gas in the far IR and submillimeter spectral ranges60 (10) (2017)
    95.30.−k, 95.85.Fm, 95.85.Gn, 97.10.Bt, 98.58.−w (all)
  2. I.V. Galaktionov “Search for antimatter and dark matter, precision studies of the cosmic rays fluxes on the international space station. AMS experiment. Results of four year exposure60 40–57 (2017)
    13.85.Tp, 14.60.−z, 29.30.−h, 75.50.Ww, 95.30.−k, 95.55.−n, 96.50.S−, 97.60.−s, 98.58.Mj, 98.70.Sa (all)
  3. S.I. Blinnikov “Mirror matter and other dark matter models57 183–188 (2014)
    12.60.−i, 95.30.−k, 95.35.+d (all)
  4. N.S. Kardashev “The radio Universe50 529–534 (2007)
    01.10.Fv, 95.30.−k, 95.55.Jz, 95.85.Bh (all)
  5. V.S. Beskin “School of modern astrophysics50 103–105 (2007)
    01.10.Fv, 95.30.−k (all)
  6. A.A. Vikhlinin, R.A. Sunyaev, E.M. Churazov “International Conference on Cosmology and High Energy Astrophysics (Zel’dovich-90) Moscow, 20-24 December 200448 533–535 (2005)
    01.10.Fv, 95.30.−k, 98.80.−k (all)
  7. V.S. Beskin “Radio pulsars42 1071 (1999)
    04.40.Dg, 95.30.−k, 97.60.Gb, 98.70.Dk (all)
  8. D.G. Yakovlev, K.P. Levenfish, Yu.A. Shibanov “Cooling of neutron stars and superfluidity in their cores42 737 (1999)
    04.40.−b, 26.60.+c, 95.30.−k, 97.60.Jd (all)
  9. Ya.M. Kramarovskii, V.P. Chechev “The puzzle of the lightest elements: observations, predictions, hypotheses42 563 (1999)
    95.30.−k, 98.80.−k, 98.80.Ft (all)
  10. D. Fargion, A. Salis “Inverse Compton scattering off black body radiation in high energy physics and gamma (MeV-TeV) astrophysics41 823–829 (1998)
    13.60.Fz, 95.30.−k, 95.85.Pw, 98.70.Rz (all)
  11. N.V. Ardelyan, G.S. Bisnovatyi-Kogan, S.G. Moiseenko “Explosion mechanisms of supernovae: the magnetorotational model40 1076–1079 (1997)
    04.40.Dg, 95.30.−k, 97.60.Bw (all)
  12. V.I. Slysh “Stars, planets, and cosmic masers40 1079–1079 (1997)
    95.30.−k
  13. M.A. Liberman, B. Johansson “Properties of matter in ultrahigh magnetic fields and the structure of the surface of neutron stars38 117–136 (1995)
    95.30.−k
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