Physics – Optics
Scientific paper
May 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..267..195b&link_type=abstract
Co-Evolution of Central Black Holes and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 267
Physics
Optics
Black Hole Physics, Galaxies: Individual (Ngc 1265), Galaxies: Elliptical And Lenticular, Cd, Galaxies: Kinematics And Dynamics, Instrumentation: Adaptive Optics
Scientific paper
We present K-band adaptive-optics assisted spectroscopic observations of the central region of the archetype head-tail radio galaxy NGC 1265 (3C 83.1), with the aim of constraining the mass of the supermassive black hole (MBH). The near-infrared data taken with the Altair-NIRI system on the Gemini North have a spatial resolution of FWHM = 0.”11 (39 pc, at the galaxy's distance of 73 Mpc).
Beifiori Alessandra
Cappellari Michele
Davies Roger L.
Houghton Ryan C. W.
Sarzi Marc
No associations
LandOfFree
Searching for the Supermassive Black Hole in NGC 1265 (3C 83.1B) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Searching for the Supermassive Black Hole in NGC 1265 (3C 83.1B), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Searching for the Supermassive Black Hole in NGC 1265 (3C 83.1B) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-793406