Sie suchten nach: galaxies (Türkisch - Englisch)

* strange setup: andromeda's satellite galaxies all lined up
*strange setup: andromeda's satellite galaxies all lined up

this is among the most massive black holes measured in any nearby galaxies.
this is among the most massive black holes measured in any nearby galaxies.

10 march 2006 gigantic cosmic cataclysm in stephan's quintet of galaxies* stephan's quintet.
10 march 2006 gigantic cosmic cataclysm in stephan's quintet of galaxies* stephan's quintet.

these results have been repeatedly used to demonstrate that thenumber of globular clusters in galaxies is thought to be related to the size of the galaxies' bulges.
these results have been repeatedly used to demonstrate that the number of globular clusters in galaxies is thought to be related to the size of the galaxies' bulges.

the ratio of the number of globular clusters to the total luminosity of the galaxy is high compared to the milky way and similar galaxies with small bulges, but the ratio is comparable to other galaxies with large bulges.
the ratio of the number of globular clusters to the total luminosity of the galaxy is high compared to the milky way and similar galaxies with small bulges, but the ratio is comparable to other galaxies with large bulges.

98* reverberation measurements of the inner radius of the dust torus in nearby seyfert 1 galaxies, suganuma et al., apj, march 2006, vol.
98*reverberation measurements of the inner radius of the dust torus in nearby seyfert 1 galaxies, suganuma et al., apj, march 2006, vol.

uppsala genel kataloğu ("uppsala general catalogue of galaxies") (ugc), kuzey yarıküreden görülebilen 12921 gökadayı içeren katalog.
the uppsala general catalogue of galaxies (ugc) is a catalogue of 12921 galaxies visible from the northern hemisphere.

: galaxy rotation problem: is dark matter responsible for differences in observed and theoretical speed of stars revolving around the center of galaxies, or is it something else?
; galaxy rotation problem: is dark matter responsible for differences in observed and theoretical speed of stars revolving around the center of galaxies, or is it something else?

== kaynaklar ==* catalogue of double and multiple galaxies, erik holmberg, 1937* a catalogue of dwarf galaxy candidates around interacting galaxies, astron.
==references==* catalogue of double and multiple galaxies, erik holmberg, 1937* a catalogue of dwarf galaxy candidates around interacting galaxies, astron.

* long-term variability of the optical emission lines in the nuclear spectrum of the seyfert galaxy ngc 3227, active galaxies newsletter, no 98, pronik i., metik l., may 2005* reverberation measurements of the inner radius of the dust torus in nearby seyfert 1 galaxies, m. suganuma et al., astrophysics journal, vol 639, march 2006== dış bağlantılar ==* glen youman's astrophotos of ngc 3226 and ngc 3227* cosmic voyages webpage on ngc 3226 and ngc 3227* spitzer observations of the interacting galaxy pair* long-term variability of the optical emission lines in the nuclear spectrum of the seyfert galaxy ngc 3227, pronik et al., active galaxies newsletter, no.
* long-term variability of the optical emission lines in the nuclear spectrum of the seyfert galaxy ngc 3227, "active galaxies newsletter", no 98, pronik i., metik l., may 2005* reverberation measurements of the inner radius of the dust torus in nearby seyfert 1 galaxies, m. suganuma et al., astrophysics journal, vol 639, march 2006==external links==*glen youman's astrophotos of ngc 3226 and ngc 3227*cosmic voyages webpage on ngc 3226 and ngc 3227*spitzer observations of the interacting galaxy pair*long-term variability of the optical emission lines in the nuclear spectrum of the seyfert galaxy ngc 3227, pronik et al., active galaxies newsletter, no.