The MBH-M* relation for X-ray-obscured, red QSOs at 1.2 < z < 2.6-Reference-Cited by-同舟云学术

The MBH-M* relation for X-ray-obscured, red QSOs at 1.2 < z < 2.6

Published:2014-07-28 Issue:3 Volume:443 Page:2077-2091
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Bongiorno A.,Maiolino R.,Brusa M.,Marconi A.,Piconcelli E.,Lamastra A.,Cano-Díaz M.,Schulze A.,Magnelli B.,Vignali C.,Fiore F.,Menci N.,Cresci G.,La Franca F.,Merloni A.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/443/3/2077/4897688/stu1248.pdf

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3. Heavily reddened quasars atz∼ 2 in the UKIDSS Large Area Survey: a transitional phase in AGN evolution

4. THE RELATION BETWEEN BLACK HOLE MASS AND HOST SPHEROID STELLAR MASS OUT TOz∼ 2

5. THE RADIUS-LUMINOSITY RELATIONSHIP FOR ACTIVE GALACTIC NUCLEI: THE EFFECT OF HOST-GALAXY STARLIGHT ON LUMINOSITY MEASUREMENTS. II. THE FULL SAMPLE OF REVERBERATION-MAPPED AGNs

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