[1] Page, L., Hinshaw, G., Komatsu, E., et al. (2007) Three year wilkinson microwave anisotropy probe observa- tions: Polarization analysis. The Astrophysical Journal Supplement Series, 170(2), 335-376.
[2] Landecker, T.L. and Wielebinski, R. (1970) The galactic metre wave radiation. Australian Journal of Physics. Astrophysical Supplement, 16, 1-20.
[3] Berkhuijsen, E.M. (1973) Galactic continuum loops and the diameter-surface brightness relation for supernova remnants. Astronomy & Astrophysics, 24, 143-147.
[4] Heiles, C. (1998) Whence the local bubble, gum, orion? Astrophysical Journal, 498, 689-703.
[5] Lallement, R., Welsh, B.Y., Vergely J.L., et al. (2003) 3D mapping of the dense interstellar gas around the local bubble. Astronomy & Astrophysics, 411(3), 447-464.
[6] Shatsova, R.B. and Anisimova, G.B. (2002) The spur system in ecliptic coordinates. Astrophysics, 45(4), 535-546.
[7] Shatsova, R.B. and Anisimova, G.B. (2003) The local system harmony. Astrophysics, 46(2), 319-329.
[8] Dolidze, M.V. (1980) Peculiarities of local spiral arm features of the Galaxy. Letters to Astronomical Journal, 6, 745-749
[9] Borka, V., Milogradov-Turin, J. and Uro?evic, D. (2008) The brightness of the galactic radio loops at 1420 MHz: some indications for the existence of loops V and VI. Astronomische Nachrichten, 329(4), 397-402.
[10] Drosdovsky, I. (2007) The local group of galaxies. http://www.astronet.ru/db/msg/1169715
[11] De Vaucouleurs, G., Val, A. and Corwin, H.G. (1976) Second reference catalogue of bright galaxies, Austin, London.
[12] Shatsova, R.B. and Anisimova, G.B. (2008) The large sky Lens. Odessa Astronomical Publications, 21, 106-107.
[13] Elmegreen, B.G. and Elmegreen, D.M. (1983) Monthly notices of the royal astronomical society, 203, 31.
[14] Efremov, Y.N. (2004) Stellar complexes and starburst cumps. Proceedings of Astrophysics and Cosmology after Gamow, Odessa, 90.
[15] Lindblad, P.O. (2000) On the rotation of Gould Belt. Astronomy & Astrophysics, 363(1), 154-158.
[16] Loktin, A.V. and Popova M.E. (2007) The vavelet-smoothed distribution of young stellar objects in the galactic plane. Astronomicheski? Zhurnal, in Russian, 84(5), 409-417.
[17] Shatsova, R.B. and Anisimova, G.B. (1997) The dynamical scheme of local system. In: Agekian, T.A., Mullari, A.A. and Orlov, V.V., Eds., Structure and Evolution of Stellar Systems, St. Peterburg University Press, 184-188.
[18] Comeron, F. (1997) The Gould Belt. In: Agekian, T.A., Mullari, A.A. and Orlov, V.V., Eds., Structure and Evolution of Stellar Systems, St. Peterburg University Press, 161-173.
[19] Hu, E. (1981) High latitude HI shells in the Galaxy.I. Astrophysical Journal, 248, 119-127.
[20] K?nyvers, V., Kiss, Cs., Moor, A., et al. (2007) Catalogue of far-infra-red loops in the Galaxy. Astronomy and Astrophysics, 463(3), 1227-1234.
[21] Popovic, G.M., Ninkovic, S. and Pavlovic, R. (1997) A kinematical approach to the separation of moving-cluster members. In: Agekian, T.A., Mullari, A.A. and Orlov, V.V., Eds., Structure and Evolution of Stellar Systems, St. Peterburg University Press, 108-113.