English

The light curves of type II-P SN 2017eaw: first 200 days

Solar and Stellar Astrophysics 2018-01-03 v1 High Energy Astrophysical Phenomena

Abstract

We present UBVRI photometry of the supernova 2017eaw in NGC 6946, obtained in the period from May 14 until December 7, 2017. We derive dates and magnitudes of maximum light in the UBVRI bands and the parameters of the light curves. We discuss colour evolution, extinction and maximum luminosity of SN 2017eaw. Preliminary modeling is carried out, and the results are in satisfactory agreement with the light curves in the UBVRI bands.

Keywords

Cite

@article{arxiv.1801.00340,
  title  = {The light curves of type II-P SN 2017eaw: first 200 days},
  author = {D. Yu. Tsvetkov and S. Yu. Shugarov and I. M. Volkov and N. N. Pavlyuk and O. V. Vozyakova and N. I. Shatsky and A. A. Nikiforova and I. S. Troitsky and Yu. V. Troitskaya and P. V. Baklanov},
  journal= {arXiv preprint arXiv:1801.00340},
  year   = {2018}
}

Comments

15 pages, 6 figures, accepted by Astronomy Letters