activity
20002026
most citedOptical and Infrared Spectroscopy of the type IIn SN 1998S : Days 3-127

206 citations · 565 across the 15 of their papers we have counts for

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astro-ph.SR2014★ 20 cited

Parameters of type IIP SN 2012A and clumpiness effects

V. P. Utrobin, N. N. Chugai

The explosion energy and the ejecta mass of a type IIP supernova (SN IIP) derived from hydrodynamic simulations are principal parameters of the explosion theory. However, the numbe…

astro-ph.SR2014★ 8 cited

Evolutionary status of the active star PZ Mon

Yu. V. Pakhomov, N. N. Chugai, N. I. Bondar +2

We use original spectra and available photometric data to recover parameters of the stellar atmosphere of PZ Mon, formerly referred as an active red dwarf. The derived effective te…

astro-ph.SR2013★ 29 cited

Type IIP supernova 2008in: the explosion of a normal red supergiant

V. P. Utrobin, N. N. Chugai

The explosion energy and the ejecta mass of a type IIP supernova make up the basis for the theory of explosion mechanism. So far, these parameters have only been determined for sev…

astro-ph.SR2012★ 11 cited

Interstellar absorptions and shocked clouds towards supernova remnant RX J0852.0-4622

Yu. V. Pakhomov, N. N. Chugai, A. F. Iyudin

We present results of survey of interstellar absorptions towards supernova remnant (SNR) RX J0852.0-4622. The distribution of KI absorbers along the distance of the background star…

astro-ph.SR2011★ 52 cited

Supernova 2000cb: high-energy version of SN 1987A

V. P. Utrobin, N. N. Chugai

Among type IIP supernovae there are a few events that resemble the well-studied supernova 1987A produced by the blue supergiant in the Large Magellanic Cloud. We study a peculiar s…

astro-ph.SR2010★ 10 cited

Search for broad absorption lines in spectra of stars in the field of supernova remnant RX J0852.0-4622 (Vela Jr.)

A. F. Iyudin, Yu. V. Pakhomov, N. N. Chugai +4

Supernova remnant (SNR) RX J0852.0-4622 is one of the youngest and is most likely the closest among known galactic supernova remnants (SNRs). It was detected in X-rays, the 44Ti ga…