Parameters of Radio Pulsars at Different Distances from the “Death Line”
Calculations of angles between magnetic moments and rotation axes have been carried out for radio pulsars located at different distances from the “death line.” We have shown that these angles decrease from 36° to 10° when pulsars move to the “death line”. Such values correspond to kinematic ages fro...
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Veröffentlicht in: | Astronomy reports 2023-11, Vol.67 (11), p.1177-1186 |
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description | Calculations of angles
between magnetic moments and rotation axes have been carried out for radio pulsars located at different distances from the “death line.” We have shown that these angles decrease from 36° to 10° when pulsars move to the “death line”. Such values correspond to kinematic ages from 1 to 10 millions of years. We also argue that radio luminosities of pulsars decrease for these ages. This means that radio pulsars fade out when their age increases. |
doi_str_mv | 10.1134/S1063772923110070 |
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between magnetic moments and rotation axes have been carried out for radio pulsars located at different distances from the “death line.” We have shown that these angles decrease from 36° to 10° when pulsars move to the “death line”. Such values correspond to kinematic ages from 1 to 10 millions of years. We also argue that radio luminosities of pulsars decrease for these ages. This means that radio pulsars fade out when their age increases.</description><subject>Astronomy</subject><subject>Kinematics</subject><subject>Magnetic moments</subject><subject>Mortality</subject><subject>Observations and Techniques</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Pulsars</subject><issn>1063-7729</issn><issn>1562-6881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><recordid>eNp1UMtOwzAQtBBIlMIHcLPEOeC1E9s5opaXFImKxzlykjVN1SbFdg_c-iHwc_0SHBWJA2IvO9qZ2V0NIefALgFEevUMTAqleM4FAGOKHZARZJInUms4jDjSycAfkxPvF4wBaCFHpJgZZ1YY0HnaW_pkmrans83SmzgwgU5ba9FhNyAfTFejp9b1KxrmSHfbzymaMKdF2-Fu-3VKjqxZejz76WPyenvzMrlPise7h8l1kdRc6pA0mTaW60rLhmeqVhWHGlljMl1lRijUqbIpA6FZlgoxvKog0qDzXDVSVmJMLvZ7165_36AP5aLfuC6eLHkO8QaLFVWwV9Wu996hLdeuXRn3UQIrh9DKP6FFD997fNR2b-h-N_9v-gbU321q</recordid><startdate>20231101</startdate><enddate>20231101</enddate><creator>Ken’ko, Z. V.</creator><creator>Malov, I. F.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20231101</creationdate><title>Parameters of Radio Pulsars at Different Distances from the “Death Line”</title><author>Ken’ko, Z. V. ; Malov, I. F.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c268t-d58af28b86d257c7b21ce0da58b5a37e847f40138054330011710da18997d66b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Astronomy</topic><topic>Kinematics</topic><topic>Magnetic moments</topic><topic>Mortality</topic><topic>Observations and Techniques</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Pulsars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ken’ko, Z. V.</creatorcontrib><creatorcontrib>Malov, I. F.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astronomy reports</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ken’ko, Z. V.</au><au>Malov, I. F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Parameters of Radio Pulsars at Different Distances from the “Death Line”</atitle><jtitle>Astronomy reports</jtitle><stitle>Astron. Rep</stitle><date>2023-11-01</date><risdate>2023</risdate><volume>67</volume><issue>11</issue><spage>1177</spage><epage>1186</epage><pages>1177-1186</pages><issn>1063-7729</issn><eissn>1562-6881</eissn><abstract>Calculations of angles
between magnetic moments and rotation axes have been carried out for radio pulsars located at different distances from the “death line.” We have shown that these angles decrease from 36° to 10° when pulsars move to the “death line”. Such values correspond to kinematic ages from 1 to 10 millions of years. We also argue that radio luminosities of pulsars decrease for these ages. This means that radio pulsars fade out when their age increases.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S1063772923110070</doi><tpages>10</tpages></addata></record> |
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subjects | Astronomy Kinematics Magnetic moments Mortality Observations and Techniques Physics Physics and Astronomy Pulsars |
title | Parameters of Radio Pulsars at Different Distances from the “Death Line” |
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