dc.contributor.author |
Sergienko M.V. |
|
dc.contributor.author |
Sokolova M.G. |
|
dc.contributor.author |
Nefedyev Y.A. |
|
dc.contributor.author |
Andreev A.O. |
|
dc.date.accessioned |
2021-02-25T20:37:14Z |
|
dc.date.available |
2021-02-25T20:37:14Z |
|
dc.date.issued |
2020 |
|
dc.identifier.issn |
1063-7729 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/162057 |
|
dc.description.abstract |
© 2020, Pleiades Publishing, Ltd. Abstract—: This study is focused on the relationships between the κ-Cygnid meteor shower and different groups of asteroids crossing the Earth’s orbit (the so-called near-Earth objects (NEOs)). The analysis is based on the visible structure of the meteor shower and a comprehensive strategy for estimating the proximity of orbits of two bodies. The κ-Cygnid meteor shower (abbreviated as KCG) is observed from August 3 to August 25 every year; it is classified as a minor shower, and the size of its mean orbit is around 3.2 AU, while the geocentric velocity is 20.9 km/s. No parent body (PB) of the shower has been found among comets so far. Relationships between the shower and asteroids, as potential PBs of the shower, are under active examination; some hypotheses on this subject can be found on the website of the Meteor Data Center (MDC) of the International Astronomical Union (IAU). |
|
dc.relation.ispartofseries |
Astronomy Reports |
|
dc.title |
The κ-Cygnid Meteor Shower and Its Relationship with Near-Earth Asteroids |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
12 |
|
dc.relation.ispartofseries-volume |
64 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
1087 |
|
dc.source.id |
SCOPUS10637729-2020-64-12-SID85098503430 |
|