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pro vyhledávání: '"Shablovinskaya, Elena"'
For type-1 active galactic nuclei (AGNs) for which the equatorial scattering is the dominant broad line polarization mechanism, it is possible to measure the supermassive black hole mass by tracing the Keplerian motion across the polarization plane p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=arXiv_______::28a4d65bb6c91b1ffbb648846920911a
http://arxiv.org/abs/2007.11475
http://arxiv.org/abs/2007.11475
For type-1 active galactic nuclei (AGNs) for which the equatorial scattering is the dominant broad line polarization mechanism, it is possible to measure the supermassive black hole mass by tracing the Keplerian motion across the polarization plane p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cbbd6a8acf143dbd367296a87f1d8565
Autor:
Malygin, Eugene, Uklein, Roman, Shablovinskaya, Elena, Perepelitsyn, Aleksander, Grokhovskaya, Aleksandra
The most popular method of the broad-line region size estimation in active galactic nuclei (AGN) is the reverberation mapping based on measuring the time delay between the continuum flux and the flux in the emission lines. In our work, we apply the m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e80d80848dd40dad7b746d0ce0ba061c
Autor:
Uklein, Roman, Malygin, Eugene, Shablovinskaya, Elena, Perepelitsyn, Aleksander, Grokhovskaya, Aleksandra
The improvement of the calibration relation for determining the size of the broad-line region from the observed optical luminosity of active galactic nuclei (AGN) is a necessary task to study fundamental parameters of distant AGNs such as mass of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5a51a6cb137a4870a3ef5a8d25d1de0b