Abell 1795

Abell 1795 is a galaxy cluster in the Abell catalogue.

Abell 1795
Observation data (Epoch J2000)
Constellation(s)	Boötes
Right ascension	13h 49m 00.5s[1]
Declination	+26° 35′ 07″[1]
Richness class	2[2]
Bautz–Morgan classification	I [2]
Redshift	0.062476 (18 730)[1]
Distance	266 Mpc (868 Mly) h−1 0.705[1]
ICM temperature	6.12 keV[3]
Binding mass	6.03×1014[3] M☉
X-ray flux	(68.10 ± 5.8%)×10−12 erg s−1 cm−2 (0.1–2.4 keV)[1]

Black holes

In January 2014, scientists using data collected by the Chandra X-Ray Observatory and other telescopes reported they had found evidence of a new supermassive black hole candidate disrupting a star in a dwarf galaxy in the Abell 1795 cluster.^[4][5]

See also

• Abell catalogue
• List of Abell clusters