What Causes the Active Galactic Nuclei of Quasars During the Quasar Epoch to be so Luminous?

Authors

  • Amaliya Atamalibekova Thornton Donovan School
  • Sanah Bhimani

DOI:

https://doi.org/10.47611/jsrhs.v11i3.2935

Keywords:

Quasar, Supermassive Black Hole, Accretion, Galaxy, Active Galactic Nucleus

Abstract

The brightest quasars were born 10 billion years ago during the Quasar Epoch. These quasars were bigger and brighter than any of the quasars formed after, and this paper seeks to find out why. Quasars are a type of Active Galactic Nucleus, which is a compact center of a galaxy. The type of galaxy that contains the Active Galactic Nucleus plays an important part in their luminosity, as elliptical galaxies have much brighter Active Galactic Nuclei than spiral galaxies. The reason that Active Galactic Nuclei form in galaxies is because galaxies contain supermassive black holes, since only supermassive black holes may contain an Active Galactic Nucleus. The stars and gas clouds present in galaxies make a bigger accretion disc. This was happening at a large rate during the Quasar Epoch as opposed to now.

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Author Biography

Sanah Bhimani

Advisor

References or Bibliography

French DK. Evolution Through the Post-Starburst Phase: Using Post-Starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution. ArXiv, 2106.05982, 2021.

Melinder J, Dahlen T, Trinchant LM, ̈Ostlin G, Mattila S, Sollerman J, Fransson C, Hayes M, Kankare E, Nasoudi-Shoar S. The rate of supernovae at redshift 0.1-1.0 – the Stockholm VIMOS Supernova Survey IV. ArXiv, 1206.6897, 2012.

Schmidt M, Schneider D, Gunn J. Spectroscopic CCD Surveys for Quasars at Large Redshift. IV. Evolution of the Luminosity Function from Quasars Detected by Their Lyman-Alpha Emission. The Astronomical Journal, doi:10.1086/117497, 1995.

Latif MA, Khochfar S, Whalen D. The Birth of Binary Direct-Collapse Black Holes. ArXiv, 2002.00983, 2020.

Cattaneo A. Quasars and galaxy formation. ArXiv, 9907335, 1999.

Chiaberge M, Capetti A, Celotti A. Understanding the nature of FR II optical nuclei: a new diagnostic plane for radio galaxies. ArXiv, 0207654, 2002.

Merrifield MR, Forbes DA, Terlevich AI. The black hole mass-galaxy age relation. Monthly Notices of the Royal Astronomical Society, doi:10.1046, 2000.

Antonucci R. Active Galactic Nuclei and Quasars: Why Still a Puzzle after 50 years? ArXiv, 1501.02001, 2015.

Bengochea GR. What do we talk about when we speak of cosmological redshift? ArXiv, 1802.02444, 2018.

Gaztanaga E. The Cosmological Constant as Event Horizon. ArXiv, 2202.00641, 2022.

Kellermann KI. The Road to Quasars. ArXiv, 1412.7867, 2014.

Haemmerl ́e L, Mayer L, Klessen RS, Hosokawa T, Madau P, Bromm V. Formation of the first stars and black holes. ArXiv, 2003.10533, 2020.

Wands D, Piattella OF, Casarini L. Physics of the Cosmic Microwave Background Radiation. ArXiv, 1504.06335, 2015.

Chluba J. Tests of the CMB temperature–redshift relation, CMB spectral distortions and why adiabatic photon production is hard. Monthly Notices of the Astronomical Society, doi:10.1093, 2014.

Nagai D. THE IMPACT OF GALAXY FORMATION ON THE SUNYAEV-ZELDOVICH EFFECT OF GALAXY CLUSTERS. ArXiv, 0512208, 2006.

Rouan D. Radiative Processes. In: Gargaud M. et al. (eds) Encyclopedia of Astrobiology, doi:10.1007, 2011.

Colbert EJM, Mushotzky RF. COMPACT X-RAY SOURCES IN NEARBY GALAXY NUCLEI. ArXiv, 9809150, 1998.

Bond HE, Schaefer GH, Gilliland RL, Holberg JB, Mason BD, Lindenblad IW, Seitz-McLeese M, Arnett WD, Demarque P, Spada F, Young PA, Barstow MA, Burleigh MR, Gudehus D. The Sirius System and its Astrophysical Puzzles: Hubble Space Telescope and Ground-Based Astrometry. ArXiv, 1703.10625, 2017.

Shields GA. A Brief History of AGN. ArXiv, 9903401, 1999.

The Correlation between Black Hole Mass and Stellar Mass for Classical Bulges and the Cores of Ellipticals. ArXiv, 2011.07216, 2020.

Ba ̃nados E, Mazzucchelli C, Momjian E, Eilers A, Wang F, Schindler J, Connor T, Andika IT, Barth AJ, Carilli C, Davies FB, Decarli R, Fan X, Farina EP, Hennawi JF, Pensabene A, Stern D, Venemans BP, Wenzl L, Yang J. The discovery of a highly accreting, radio-loud quasar at z = 6.82. ArXiv, 2103.03295, 2021.

Low FJ, Schneider G. High Spatial Resolution HST/NICMOS Observations of Markarian 231. ArXiv, 0407406, 2004.

Published

08-31-2022

How to Cite

Atamalibekova, A., & Bhimani, S. (2022). What Causes the Active Galactic Nuclei of Quasars During the Quasar Epoch to be so Luminous?. Journal of Student Research, 11(3). https://doi.org/10.47611/jsrhs.v11i3.2935

Issue

Section

HS Review Articles