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High resolution studies of the IDV quasar J1128+592
Gabanyi, Krisztina Eva1,2; Marchili, Nicola3; Krichbaum, Thomas3; Fuhrmann, Lars3; Liu, Xiang4; Song, Hua-Gang4
2010-03-01
Conference Name5th Workshop of Young Researchers in Astronomy and Astrophysics
Source PublicationJournal of Physics: Conference Series 218 (2010) 012013
Volume218
Pages12013
Conference DateSEP 02-04, 2009
Correspondent Emailgabanyik@sgo.fomi.hu
Conference PlaceEotvos Univ, Budapest, HUNGARY
CountryHungary
Author of SourceForgacsDajka, E ; Plachy, E ; Molnar, L
Publication PlaceDIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND
PublisherInstitute of Physics Publishing
Contribution Rank4
AbstractJ1128+592 is a compact radio quasar and, as 30% of flat spectrum radio sources, shows fast variations in the cm-wavelength regime on time-scales of an hour to few days. Such phenomenon is often explained by scattering of radio waves in the turbulent, ionized interstellar matter of the Milky Way. Regular monitoring observations of J1128+592 performed by the Effelsberg 100-meter and the Urumqi 25-meter radio telescope during the last four years confirmed this, since a seasonal cycle of the variability time-scale was revealed. This effect is one of the most convincing argument in favor of the interstellar scattering induced fast radio variations in blazars. Multi-epoch, multi-frequency observations made by the Very Long Baseline Array (VLBA) together with the annual modulation model enabled us to determine a lower limit of the distance of the screen responsible for the rapid variability. Additionally, it revealed source-intrinsic-change, which affected the variability pattern. 2010 IOP Publishing Ltd.
KeywordAstrophysics Radio astronomy Telescopes Blazars High resolution Interstellar matter Long baseline array Lower limits Milky ways Modulation models Multi frequency ON time Radio sources Seasonal cycle Time-scales Variability patterns Wavelength regimes
DOI10.1088/1742-6596/218/1/012013
URL查看原文
Indexed ByEI ; CPCI
Language英语
ISSN1742-6588;1742-6596
WOS IDWOS:000287785100013
EI Accession Number20102913087891
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Document Type会议论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/3139
Collection射电天文研究室_星系宇宙学研究团组
科研仪器设备产出_利用南山26米射电望远镜(NSRT)观测数据的文章
Corresponding AuthorGabanyi, Krisztina Eva
Affiliation1.FOMI Satellite Geodetic Observatory, Budapest, P.O.Box 585 1592 Hungary;
2.Hungarian Academy of Sciences, Research Group for Physical Geodesy and Geodynamics, Budapest, Hungary;
3.Max-Planck-Institute f¨ur Radioastronomie, Auf dem H¨ugel 69, Bonn 53121 Germany;
4.Urumqi Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Urumqi 830011, PR China
Recommended Citation
GB/T 7714
Gabanyi, Krisztina Eva,Marchili, Nicola,Krichbaum, Thomas,et al. High resolution studies of the IDV quasar J1128+592[C]//ForgacsDajka, E, Plachy, E, Molnar, L. DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND:Institute of Physics Publishing,2010:12013.
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