The S4G Sample: Absorption Properties of AGNs by WISE, 3XMM, and FIRST/NVSS
Öz
Anahtar Kelimeler
Kaynakça
- Best, P. N., Heckman T. M., 2012. On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties, Monthly Notices of the Royal Astronomical Society, 421, 1569.
- Caputi, K. I., 2014. Active galactic nuclei and their role in galaxy evolution: The infrared perspective, International Journal of Modern Physics D, 23, 1430015.
- Elvis M. et al., 1994. Atlas Of Quasar Energy Distributions, The Astrophysical Journal Supplement Series, 95:1-68.
- Fabian, A. C., Iwasawa K., 1999,. The mass density in black holes inferred from the X-ray background, Monthly Notices of the Royal Astronomical Society, 303, L34.
- Ferrarese, L. & Merritt, D. 2000. A Fundamental Relation Between Supermassive Black Holes And Their Host Galaxies, The Astrophysical Journal, 539:L9–L12.
- Gebhardt K., et al., 2000. A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion, The Astrophysical Journal, 539, L13.
- Hardcastle, M. J., Evans D. A., Croston J. H., 2009. The active nuclei of z < 1.0 3CRR radio sources, Monthly Notices of the Royal Astronomical Society, 396, 1929.
- Hasinger, G., 2018. Absorption properties and evolution of active galactic nuclei, Astronomy and Astrophysics, 490, 905-922.
Ayrıntılar
Birincil Dil
İngilizce
Konular
Mühendislik
Bölüm
Araştırma Makalesi
Yazarlar
Tuba İkiz
*
0000-0003-4085-6287
Türkiye
Yayımlanma Tarihi
31 Ağustos 2021
Gönderilme Tarihi
8 Haziran 2021
Kabul Tarihi
31 Ağustos 2021
Yayımlandığı Sayı
Yıl 2021 Cilt: 14 Sayı: 2