A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Optical Photometric and Radio Monitoring of Gamma-ray Loud Blazars
Tekijät: Bychkova VS, Kardashev NS, Larionov MG, Volvach AE, Vlasjuk VV, Spiridonova OI, Lachteenmaki A, Tornikoski M, Hovatta T, Nieppola E, Torniainen I, Aller HD, Aller MF
Kustantaja: INDIAN ACAD SCIENCES
Julkaisuvuosi: 2011
Lehti: Journal of Astrophysics and Astronomy
Tietokannassa oleva lehden nimi: JOURNAL OF ASTROPHYSICS AND ASTRONOMY
Lehden akronyymi: J ASTROPHYS ASTRON
Vuosikerta: 32
Numero: 1-2
Aloitussivu: 105
Lopetussivu: 108
Sivujen määrä: 4
ISSN: 0250-6335
DOI: https://doi.org/10.1007/s12036-011-9015-6
Tiivistelmä
The harmonic analysis performed for the light curves of 0716+714 from 2002-2010 in radio and optical wave bands revealed the presence of an apparent periodical component in the flux variations. The period of the radio light curve is nearly 3.6 years, and coincides within the errors with the period of the optical light curve (nearly 3.4 years). The duration of the flares is approximately the same in radio and optical ranges, and it is about 100-150 days.
The harmonic analysis performed for the light curves of 0716+714 from 2002-2010 in radio and optical wave bands revealed the presence of an apparent periodical component in the flux variations. The period of the radio light curve is nearly 3.6 years, and coincides within the errors with the period of the optical light curve (nearly 3.4 years). The duration of the flares is approximately the same in radio and optical ranges, and it is about 100-150 days.
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