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 961–993 (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)
  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)
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