THE HISTOGRAM OF PULSARS' PERIODS DISTRIBUTION

V. P. Bezdenezhnyi

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.

Ключові слова


Stars; pulsars; δ Scuti; RR Lyrae; classical Cepheids; bimodal Cepheids; β Cep stars.

Повний текст:

PDF (English)

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.




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

Посилання

  • Поки немає зовнішніх посилань.


Copyright (c) 2017 Odessa Astronomical Publications

Creative Commons License
Ця робота ліцензована Creative Commons Attribution-NonCommercial 4.0 International License.