Vigen Malumian

Vigen Malumian (Armenian: Վիգեն Հայկի Մալումյան) (Russian: Виген Гайкович Малумян) (11 March 1932 – 2 February 2013) was an Armenian astrophysicist who specialised in radio galaxies and the radio characteristics of spiral galaxies. He was a prominent scientist at the Byurakan Observatory in Armenia (BAO), a professor at the Faculty of Physics at Yerevan State University, and a member of the BAO Scientific Board.

Malumian died in Yerevan on 2 February 2013, at the age of 80.

Works GPS and CSS radio sources

Relationship Between Infrared and Radio Emission of Spiral Galaxies

Activity Phenomena Observed at Radio Frequences in Spiral Galaxies

Radio luminosity of spiral galaxies

Relationship between radio luminosity and optical surface brightness of spiral galaxies

Radio Emission Spectra of Isolated Spiral Galaxies and Spiral Members of Pairs of Galaxies

On the question of radio emission of spiral galaxies in groups of galaxies

On the Radio Emission of Spiral Galaxies in Double System of Galaxies

Radio Spectrum and Surface Brightness of Radio Galaxies

Observations of faint radio galaxies with the RATAN-600 radio telescope

Radio luminosities and structure of central regions of spiral galaxies

Radio emission of elliptical and lenticular galaxies in groups of galaxies

On Enhanced Radio Emission of Spiral Components of Double Galaxies and of Groups of Galaxies

RATAN-600 Observations of Faint Bologna Radio Galaxies at 7.6-CM and 3.9-CM

Radio Emission of Spiral Galaxies in Groups of Galaxies

On the Radio Emission from Interacting Spiral Galaxies

Radio emission of isolated single and double galaxies

RATAN-600 Observations of another 15 Bologna Radio Galaxies

Colors and the Byurakan classification of galaxies

RATAN-600 Observations of 15 Bologna Radio Galaxies

Investigation of galaxies of high surface brightness at 3.95 GHz

Radio Spectra and the Byurakan Classification of Galaxies

On the variability of the radio emission of Markarian 421

Observations of Galaxies of High Surface Brightness at 3.66-GHZ - Part One

Optical Surface Brightnesses and Radio Luminosities of Galaxies

Observations of Galaxies of High Surface Brightness with the Radio Telescope RATAN-600

The break in the radio emission spectrum of Cassiopeia A

Radio emission of the galactic nucleus

The Radio Spectrum of the Galactic Nucleus

Observations of Galactic Plane Near delta = -24deg23' at Wavelength 32.5 cm with High Resolving Power

Results of observations of Omega (NGC 6618) nebula made with the large Pulkovo radio telescope at wavelength 32.5 cm

The Results of the Observations of Radio Source Sagittarius-A at 32.5 cm Wavelength with High Resolution Power

Observation of the Region near the Galactic Center on a Wavelength of 33.3 cm with the Large GAO Radio Telescope