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Search of the radio emission from flare stars at decameter wavelengths

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dc.contributor.author Boiko, A.I.
dc.contributor.author Konovalenko, A.A.
dc.contributor.author Koliadin, V.L.
dc.contributor.author Melnik, V.N.
dc.date.accessioned 2017-06-04T18:55:57Z
dc.date.available 2017-06-04T18:55:57Z
dc.date.issued 2012
dc.identifier.citation Search of the radio emission from flare stars at decameter wavelengths / A.I. Boiko, A.A. Konovalenko, V.L. Koliadin, V.N. Melnik // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 121-124. — Бібліогр.: 11 назв. — англ. uk_UA
dc.identifier.issn 2227-1481
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119179
dc.description.abstract Observations of the two M-dwarf flare stars (AD Leonis and EV Lacertae), which were carried out with the radio telescope UTR-2 (Kharkiv, Ukraine) in the range of 16.5 − 33 MHz, are presented. 167 events of radio emission from AD Leo and 73 events from EV Lac were detected in the period of 2010-2011. These events were considered as stellar emission in ON-OFF regime of observations. The morphology of the probable events in the form of bursts from flare stars is considered and frequency drift rates, durations and uxes of the bursts are analysed. uk_UA
dc.description.sponsorship The work was partly supported by SOLSPANET project and authors are grateful to Stefaan Poedts for discussion of observational results. uk_UA
dc.language.iso en uk_UA
dc.publisher Головна астрономічна обсерваторія НАН України uk_UA
dc.relation.ispartof Advances in Astronomy and Space Physics
dc.title Search of the radio emission from flare stars at decameter wavelengths uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA


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