supermassive black hole

Select : aas active galactic nucleus ALMA anniversary ARDC asteroid asteroids astrophotography astrophotography workshop Atacama Atacama Large Millimeter/submillmeter array AUI aui program AUI Scholarship awards baseline binary binary stars birth black hole black holes blazar Broader Impacts brown dwarf Caltech casa CDL census Central Development Laboratory Cepheus a cfa chandra coma berenices Coma cluster comets cosmic cosmic explosion cosmicai cosmology cryo CSO dark matter dead galaxy Decadal Survey deep field deep field imaging dftau digital backend distant galaxy diversity dust early universe EHT EMS equity event exoplanet exoplanets fast radio burst Fast Radio Bursts first fringes flare fotau frb fringes funding galaxies galaxies merger galaxy galaxy cluster galex gamma ray burst gamma ray bursts gbo gbt gravitational lens gravitational waves grb grbs green bank observatory green bank telescope H20 HAM Radio helical magnetic field honors Hubble Hughes hvac hw2 hydrogen hydrogen bubble image contest inclusion international women's day Io irya Jansky Fellowships Jansky Lecture jet jet collimation jets Jupiter learning center Leroy LGBT local oscillator low noise amplifier m83 M87 magnetar Magnetars magnetic fields maser Milky Way modulus molecular clouds mou mtex NAC nasa National Astronomy Consortium National Science Foundation near earth objects nebula NEOs neutron stars neutron-star merger nglc ngVLA NINE NM noirlab nrao NRQZ NSF NSF NRAO ODI open house Orion Orion nebula parkes radio observatory pawsey people PHANGS photography planetary defense Planetary Radar planetary science plasma Postdoctoral research PRIDE protoplanetary disk protoplanets protostar protostars protostellar jet PROVOCA proxima centauri pulsar qorvo quasar radar radio telescope ram pressure stripping raytheon receiver receiver upgrade relativistic jet REU rixindustries Schinnerer scholarship science cases SETI sgrA sky survey SMBH sofia software Solar System spectrum spiral galaxies star death star factory star formation starbirth stars stellar flare stellar nurseries STEM stem ed summer research supermassive black hole supernova supernova remnant supernovae survey tde tidal disruption events trades tradesmen unam unm upgrade usno very large array very long baseline array via VLA vla open house vlass VLBA vlbi vnda water wise workshop xka xray

Radio Black Hole Trio Lights Up in Rare Galaxy Merger

Astronomers from the U.S. Naval Research Laboratory (NRL), in conjunction with scientists from the U.S. Naval Observatory (USNO) and NASA Goddard Space Flight Center (NASA GSFC), using U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) instruments have confirmed the first known triple system in which all three galaxies host actively feeding, radio-bright supermassive black holes.

The National Radio Astronomy Observatory is a facility of the U.S. National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
	Founded in 1956, the NRAO provides state-of-the-art radio telescope facilities for use by the international scientific community. NRAO telescopes are open to all astronomers regardless of institutional or national affiliation. Observing time on NRAO telescopes is available on a competitive basis to qualified scientists after evaluation of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time. NRAO also provides both formal and informal programs in education and public outreach for teachers, students, the general public, and the media.
	The U.S. National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 "to promote the progress of science; to advance the national health, prosperity, and welfare; to secure the national defense..."
	AUI collaborates with the scientific community and research sponsors to plan, build, and operate cutting-edge facilities. We cultivate excellence, deliver value, enhance education, and engage the public.