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Cold quasar

From Wikipedia, the free encyclopedia

A cold quasar is a rare population of luminous unobscured quasars associated with starburst galaxies with an high rate of star formation of about 1000 solar masses per year. Theses quasars have a significant amount of cold gas at the center of the galaxy.[1] Theses rare types of quasars are not well explained by simplistic models of quasar evolution and fueling.[2]

There are 64 galaxies that are described to host a cold quasar.[1][2]

Discovery

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The discovery of cold quasars was formally announced in 2019 by Professor Allison Kirkpatrick at the 234th meeting of the American Astronomical Society in St. Louis.[3]

References

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  1. ^ a b academic.oup.com https://academic.oup.com/mnras/article/528/4/7376/7610919. Retrieved 2024-05-14. {{cite web}}: Missing or empty |title= (help)
  2. ^ a b "Cold Quasars". kirkpatrick.ku.edu. Retrieved 2024-05-14.
  3. ^ "AAS 234 Press Conference: Cold Quasars & Hot Cosmology". AAS Press Office via YouTube. 12 June 2019. Retrieved 13 June 2019.