Add to ORKGSupermassive black hole accretion and star formation appear intimately connected. I review the observational and theoretical evidence for this statement. I then discuss how focussed studies of two systems, our Galactic Center and the nucleus of M87, can help to improve our understanding of these processes
We derive the growth of SMBHs relative to the stellar content of their host galaxy predicted under t...
In this paper we discuss the evolution of gravitationally unstable pre-galactic discs that result fr...
Galaxies grow their supermassive black holes in concert with their stars, although the relationship ...
Supermassive black holes in the centers of giant elliptical galaxies are remarkably faint given thei...
Detailed high-resolution observations of the innermost regions of nearby galaxies have revealed the ...
We review theoretical and observational arguments favoring a scenario in which a typical massive bla...
The luminosities of the centres of nearby elliptical galaxies are very low compared to models of thi...
Using X-ray stacking analyses we estimate the average amounts of supermassive black hole (SMBH) grow...
Supermassive black holes, with masses more than a million times that of the Sun, seem to inhabit the...
We study the nuclear (AGN) activity in the local Universe (z < 0.33) and its correlation with the...
none12siPrevious studies suggest that the growth of supermassive black holes (SMBHs) may be fundamen...
The existence of young stars in the central parsec of the Milky Way’s Galactic Center (GC) is challe...
Black holes (BHs) are a very important class of astrophysical objects. They are the most compact obj...
The presence of young massive stars orbiting on eccentric rings within a few tenths of a parsec of t...
While supermassive black-holes are known to co-evolve with their host galaxy, the precise nature and...
We derive the growth of SMBHs relative to the stellar content of their host galaxy predicted under t...
In this paper we discuss the evolution of gravitationally unstable pre-galactic discs that result fr...
Galaxies grow their supermassive black holes in concert with their stars, although the relationship ...
Supermassive black holes in the centers of giant elliptical galaxies are remarkably faint given thei...
Detailed high-resolution observations of the innermost regions of nearby galaxies have revealed the ...
We review theoretical and observational arguments favoring a scenario in which a typical massive bla...
The luminosities of the centres of nearby elliptical galaxies are very low compared to models of thi...
Using X-ray stacking analyses we estimate the average amounts of supermassive black hole (SMBH) grow...
Supermassive black holes, with masses more than a million times that of the Sun, seem to inhabit the...
We study the nuclear (AGN) activity in the local Universe (z < 0.33) and its correlation with the...
none12siPrevious studies suggest that the growth of supermassive black holes (SMBHs) may be fundamen...
The existence of young stars in the central parsec of the Milky Way’s Galactic Center (GC) is challe...
Black holes (BHs) are a very important class of astrophysical objects. They are the most compact obj...
The presence of young massive stars orbiting on eccentric rings within a few tenths of a parsec of t...
While supermassive black-holes are known to co-evolve with their host galaxy, the precise nature and...
We derive the growth of SMBHs relative to the stellar content of their host galaxy predicted under t...
In this paper we discuss the evolution of gravitationally unstable pre-galactic discs that result fr...
Galaxies grow their supermassive black holes in concert with their stars, although the relationship ...