activity
19962017
most citedThe supernova rate per unit mass

546 citations · 1.2k across the 33 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2017★ 24 cited

Supernovae and their host galaxies - V. The vertical distribution of supernovae in disc galaxies

A. A. Hakobyan, L. V. Barkhudaryan, A. G. Karapetyan +6

We present an analysis of the height distributions of the different types of supernovae (SNe) from the plane of their host galaxies. We use a well-defined sample of 102 nearby SNe…

astro-ph.GA2017

The Distribution of Supernovae Relative to Spiral Arms of Host Disc Galaxies

L. S. Aramyan, A. A. Hakobyan, A. R. Petrosian +7

Using a sample of 215 supernovae (SNe), we analyse their positions relative to the spiral arms of their host galaxies, distinguishing grand-design (GD) spirals from non-GD (NGD) ga…

astro-ph.GA2016

Supernovae Distribution and Host Galaxy Properties

A. A. Hakobyan, A. G. Karapetyan, L. V. Barkhudaryan +6

We present the summary of our last results on the spatial distribution and relative frequencies of Supernovae (SNe) in a large number of host galaxies from the Sloan Digital Sky Su…

astro-ph.GA2016

The Impact of Bulges on the Radial Distribution of Supernovae in Disc Galaxies

A. A. Hakobyan, A. G. Karapetyan, L. V. Barkhudaryan +6

We present the results of the analysis of the impact of bulges on the radial distributions of the different types of supernovae (SNe) in the stellar discs of host galaxies with var…

astro-ph.GA2016

The impact of bars on the radial distribution of supernovae in disc galaxies

A. A. Hakobyan, A. G. Karapetyan, L. V. Barkhudaryan +6

We present an analysis of the impact of bars on the radial distributions of the different types of supernovae (SNe) in the stellar discs of host galaxies with various morphologies.…

astro-ph.GA2016★ 33 cited

Supernovae and their host galaxies - IV. The distribution of supernovae relative to spiral arms

L. S. Aramyan, A. A. Hakobyan, A. R. Petrosian +7

Using a sample of 215 supernovae (SNe), we analyze their positions relative to the spiral arms of their host galaxies, distinguishing grand-design (GD) spirals from non-GD (NGD) ga…