Titlebook: ;

estradiol

書目名稱Growing Black Holes: Accretion in a Cosmological Context影響因子(影響力)




書目名稱Growing Black Holes: Accretion in a Cosmological Context影響因子(影響力)學(xué)科排名




書目名稱Growing Black Holes: Accretion in a Cosmological Context網(wǎng)絡(luò)公開度




書目名稱Growing Black Holes: Accretion in a Cosmological Context網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Growing Black Holes: Accretion in a Cosmological Context被引頻次




書目名稱Growing Black Holes: Accretion in a Cosmological Context被引頻次學(xué)科排名




書目名稱Growing Black Holes: Accretion in a Cosmological Context年度引用




書目名稱Growing Black Holes: Accretion in a Cosmological Context年度引用學(xué)科排名




書目名稱Growing Black Holes: Accretion in a Cosmological Context讀者反饋




書目名稱Growing Black Holes: Accretion in a Cosmological Context讀者反饋學(xué)科排名

Detonate

The Environmental Impact of Supermassive Black Holes,inciple of ., by which supermassive black holes grow until they release sufficient energy to unbind the gas that feeds them from their host galaxy. This principle explains several observed facts, including the correlation between the mass of a central black hole and the depth of the gravitational po

Contracture

The Growth of the Earliest Supermassive Black Holes and Their Contribution to Reionization,ing black holes (BHs) can help explain these observations. We show new evidence, based on the combined statistics of Lyman . and . absorption in quasar spectra, that the IGM contains a significant amount of neutral hydrogen, and is experiencing rapid ionization at redshift .~ 6. However, we argue th

Fecal-Impaction

頭腦冷靜

floaters

,Calibrating the Galaxy Halo – Black Hole Relation Based on the Clustering of Quasars,asars. The slow evolution of the clustering length with redshift inferred in the 2dF quasar redshift survey strongly favors a scenario where the central black-holes comprise a larger fraction of the host galaxy mass at higher redshifts. In a scenario where quasars are triggered by halo mergers, this

floaters

Barter

A Physically Motivated Toy Model for the BH-Spheroid Coevolution,co-evolution of massive black holes (MBHs) at the center of stellar spheroids and their stellar and gaseous components. We consider cosmological infall of gas as well as the mass and energy return for the evolving stellar population. The AGN . heating and cooling are described by assuming photoioniz

固定某物

放氣