THE HISTOGRAM OF PULSARS' PERIODS DISTRIBUTION

Автор(и)

  • V. P. Bezdenezhnyi Department of Astronomy, Odessa State University T.G.Shevchenko Park, Odessa 65014 Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2004.17.93205

Ключові слова:

Stars, pulsars, &#948, Scuti, RR Lyrae, classical Cepheids, bimodal Cepheids, &#946, Cep stars.

Анотація

In considering of the distribution of periods for pulsars taken from Smith (1979) and GCVS (1976) 20 peaks are found: at 0.672 sec, 0.450 sec, 0.403 sec, 0.270 sec, 0.191 sec and other smaller peaks. Identifications and comparison with the distribution of periods for δ Sct and β Cep stars are carried out.

Посилання

Bezdenezhnyi V.P.: 1994a, Odessa Astron. Publ., 7, 55.

Bezdenezhnyi V.P.: 1994b, Odessa Astron. Publ., 7, 57.

Bezdenezhnyi V.P.: 1997, Odessa Astron. Publ., 10, 95.

Kukarkin B.V., Kholopov P.N. et al.: 1976, Third Supplement to the third edition of the General Catalogue of Variable Stars, Nauka, Moscow, 324.

Smith F.G.: 1979, Pulsars, Moscow, 256.

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Опубліковано

2017-03-15

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