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pro vyhledávání: '"M., Urry C."'
Autor:
F., Ricci, E., Treister, E., Bauer F., E., Mejía-Restrepo J., M., Koss, S., den Brok, M., Baloković, R., Bär, P., Bessiere, T., Caglar, F., Harrison, K., Ichikawa, D., Kakkad, I., Lamperti, R., Mushotzky, K., Oh, C., Powell M., C., Privon G., C., Ricci, R., Riffel, F., Rojas A., E., Sani, L., Smith K., D., Stern, B., Trakhtenbrot, M., Urry C., S., Veilleux
Virial black hole mass ($M_{BH}$) determination directly involves knowing the broad line region (BLR) clouds velocity distribution, their distance from the central supermassive black hole ($R_{BLR}$) and the virial factor ($f$). Understanding whether
Externí odkaz:
http://arxiv.org/abs/2111.13720
Autor:
Fiona A. Harrison, Enrico Piconcelli, Sylvain Veilleux, Luca Zappacosta, Richard F. Mushotzky, A. Tortosa, Federica Ricci, Ahmed Elagali, Benny Trakhtenbrot, D. Kakkad, Claudio Ricci, K. K. Gupta, Kyuseok Oh, T. Kawamuro, Michael Koss, C. M. Urry, Turgay Caglar, M. C. Powell, Yoshihiro Ueda, Franz E. Bauer, Kohei Ichikawa, D. Stern, George C. Privon
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 504(1), 428-443
Accreting supermassive black holes (SMBHs), also known as active galactic nuclei (AGN), are generally surrounded by large amounts of gas and dust. This surrounding material reprocesses the primary X-ray emission produced close to the SMBH and gives r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a6e65e40b58ad2334e9e66d03889ccc
http://hdl.handle.net/11585/856472
http://hdl.handle.net/11585/856472