Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz
There are some known theoretical models used for investigations of pulsars at present. One of the most important parameters for the check of existing pulsar models is the angle β between an axis of an emission cone (a direction of a magnetic moment vector) and a pulsar rotation axis. Some results of...
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| Veröffentlicht in: | Advances in Astronomy and Space Physics |
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| Datum: | 2011 |
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| Format: | Artikel |
| Sprache: | English |
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Advances in astronomy and space physics
2011
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/118941 |
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| Zitieren: | Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz / E.B. Nikitina, I.F. Malov // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 2. — С. 9-12. — Бібліогр.: 3 назв. — англ. |
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Nikitina, E.B. Malov, I.F. 2017-06-01T15:02:37Z 2017-06-01T15:02:37Z 2011 Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz / E.B. Nikitina, I.F. Malov // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 2. — С. 9-12. — Бібліогр.: 3 назв. — англ. 987-966-439-367-3 https://nasplib.isofts.kiev.ua/handle/123456789/118941 There are some known theoretical models used for investigations of pulsars at present. One of the most important parameters for the check of existing pulsar models is the angle β between an axis of an emission cone (a direction of a magnetic moment vector) and a pulsar rotation axis. Some results of calculations of this angle are presented. For such calculations the sample of pulsars from the paper of Van Ommen, Alessandro et al. (1997) was used. The estimations of the angle β was carried out in three ways. The first two ways are based on some statistical relationships. The third way uses observable values of positional angles and shapes of average profiles for individual pulsars only. The distributions of angles β obtained by three methods and some results of their comparison are discussed. en Advances in astronomy and space physics Advances in Astronomy and Space Physics Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz |
| spellingShingle |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz Nikitina, E.B. Malov, I.F. |
| title_short |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz |
| title_full |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz |
| title_fullStr |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz |
| title_full_unstemmed |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz |
| title_sort |
estimations of angles between some axes in radio pulsars from catalog at 1000 mhz |
| author |
Nikitina, E.B. Malov, I.F. |
| author_facet |
Nikitina, E.B. Malov, I.F. |
| publishDate |
2011 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Advances in astronomy and space physics |
| format |
Article |
| description |
There are some known theoretical models used for investigations of pulsars at present. One of the most important parameters for the check of existing pulsar models is the angle β between an axis of an emission cone (a direction of a magnetic moment vector) and a pulsar rotation axis. Some results of calculations of this angle are presented. For such calculations the sample of pulsars from the paper of Van Ommen, Alessandro et al. (1997) was used. The estimations of the angle β was carried out in three ways. The first two ways are based on some statistical relationships. The third way uses observable values of positional angles and shapes of average profiles for individual pulsars only. The distributions of angles β obtained by three methods and some results of their comparison are discussed.
|
| isbn |
987-966-439-367-3 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/118941 |
| citation_txt |
Estimations of angles between some axes in radio pulsars from catalog at 1000 MHz / E.B. Nikitina, I.F. Malov // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 2. — С. 9-12. — Бібліогр.: 3 назв. — англ. |
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2025-11-27T09:23:52Z |
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2025-11-27T09:23:52Z |
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