PRINCE, Raj, Michal ZAJAČEK, Bozena CZERNY, Piotr TRZCIONKOWSKI, Mateusz BRONIKOWSKI, Catalina Sobrino FIGAREDO, Swayamtrupta PANDA, Mary Loli MARTINEZ-ALDAMA, Krzysztof HRYNIEWICZ, Vikram Kumar JAISWAL, Marzena SNIEGOWSKA, Mohammad-Hassan NADDAF, Maciej BILICKI, Martin HAAS, Marek Jacek SARNA, Vladimir KARAS, Aleksandra OLEJAK, Robert PRZYLUSKI, Mateusz RALOWSKI, Andrzej UDALSKI, Ramotholo R SEFAKO, Anja GENADE a Hannah L WORTERS. Wavelength-resolved reverberation mapping of quasar CTS C30.10: Dissecting Mg II and Fe II emission regions. Astronomy & Astrophysics. EDP Sciences, 2022, roč. 667, November, s. 1-20. ISSN 0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361/202243194.
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Základní údaje
Originální název Wavelength-resolved reverberation mapping of quasar CTS C30.10: Dissecting Mg II and Fe II emission regions
Autoři PRINCE, Raj, Michal ZAJAČEK (703 Slovensko, domácí), Bozena CZERNY, Piotr TRZCIONKOWSKI, Mateusz BRONIKOWSKI, Catalina Sobrino FIGAREDO, Swayamtrupta PANDA, Mary Loli MARTINEZ-ALDAMA, Krzysztof HRYNIEWICZ, Vikram Kumar JAISWAL, Marzena SNIEGOWSKA, Mohammad-Hassan NADDAF, Maciej BILICKI, Martin HAAS, Marek Jacek SARNA, Vladimir KARAS, Aleksandra OLEJAK, Robert PRZYLUSKI, Mateusz RALOWSKI, Andrzej UDALSKI, Ramotholo R SEFAKO, Anja GENADE a Hannah L WORTERS.
Vydání Astronomy & Astrophysics, EDP Sciences, 2022, 0004-6361.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Francie
Utajení není předmětem státního či obchodního tajemství
WWW URL URL
Impakt faktor Impact factor: 6.500
Kód RIV RIV/00216224:14310/22:00129257
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.1051/0004-6361/202243194
UT WoS 000879223700001
Klíčová slova anglicky accretion; accretion disks; quasars: emission lines; quasars: individual: CTS C30.10; techniques: spectroscopic; techniques: photometric
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 20. 1. 2023 14:14.
Anotace
Context. We present the results of the reverberation monitoring of the Mg II broad line and Fe II pseudocontinuum for the luminous quasar CTS C30.10 (z = 0.90052) with the Southern African Large Telescope in 2012–2021. Aims. We aimed at disentangling the Mg II and UV Fe II variability and the first measurement of UV Fe II time delay for a distant quasar. Methods. We used several methods for the time-delay measurements and determined the Fe II and Mg II time delays. We also performed a wavelength-resolved time delay study for a combination of Mg II and Fe II in the 2700–2900 Å rest-frame wavelength range. Results. We obtain a time delay for Mg II of 275.5−19.5+12.4 days in the rest frame, and we have two possible solutions of 270.0−25.3+13.8 days and 180.3−30.0+26.6 in the rest frame for Fe II. Combining this result with the old measurement of Fe II UV time delay for NGC 5548, we discuss for first time the radius-luminosity relation for UV Fe II with the slope consistent with 0.5 within the uncertainties. Conclusions. Because the Fe II time delay has a shorter time-delay component but the lines are narrower than Mg II, we propose that the line-delay measurement is biased toward the part of the broad line region (BLR) facing the observer. The bulk of the Fe II emission may arise from the more distant BLR region, however, the region that is shielded from the observer.
Návaznosti
GX21-13491X, projekt VaVNázev: Zkoumání žhavého vesmíru a porozumění kosmické zpětné vazbě (Akronym: EHU)
Investor: Grantová agentura ČR, Exploring the Hot Universe and Understanding Comic Feedback
VytisknoutZobrazeno: 24. 8. 2024 18:11