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Light Curves of the Type II-P Supernova SN 2017eaw : The First 200 Days. / Tsvetkov, D. Yu; Shugarov, S. Yu; Volkov, I. M.; Pavlyuk, N. N.; Vozyakova, O. V.; Shatsky, N. I.; Nikiforova, A. A.; Troitsky, I. S.; Троицкая, Юлия Вячеславовна; Baklanov, P. V.

In: Astronomy Letters, Vol. 44, No. 5, 01.05.2018, p. 315-323.

Research output: Contribution to journal › Article › peer-review

Harvard

Tsvetkov, DY, Shugarov, SY, Volkov, IM, Pavlyuk, NN, Vozyakova, OV, Shatsky, NI, Nikiforova, AA, Troitsky, IS, Троицкая, ЮВ & Baklanov, PV 2018, 'Light Curves of the Type II-P Supernova SN 2017eaw: The First 200 Days', Astronomy Letters, vol. 44, no. 5, pp. 315-323. https://doi.org/10.1134/S1063773718050043

APA

Tsvetkov, D. Y., Shugarov, S. Y., Volkov, I. M., Pavlyuk, N. N., Vozyakova, O. V., Shatsky, N. I., Nikiforova, A. A., Troitsky, I. S., Троицкая, Ю. В., & Baklanov, P. V. (2018). Light Curves of the Type II-P Supernova SN 2017eaw: The First 200 Days. Astronomy Letters, 44(5), 315-323. https://doi.org/10.1134/S1063773718050043

Vancouver

Tsvetkov DY, Shugarov SY, Volkov IM, Pavlyuk NN, Vozyakova OV, Shatsky NI et al. Light Curves of the Type II-P Supernova SN 2017eaw: The First 200 Days. Astronomy Letters. 2018 May 1;44(5):315-323. https://doi.org/10.1134/S1063773718050043

Author

Tsvetkov, D. Yu ; Shugarov, S. Yu ; Volkov, I. M. ; Pavlyuk, N. N. ; Vozyakova, O. V. ; Shatsky, N. I. ; Nikiforova, A. A. ; Troitsky, I. S. ; Троицкая, Юлия Вячеславовна ; Baklanov, P. V. / Light Curves of the Type II-P Supernova SN 2017eaw : The First 200 Days. In: Astronomy Letters. 2018 ; Vol. 44, No. 5. pp. 315-323.

BibTeX

@article{ca4b53b61f40498e87ef2a791f52ef26,
title = "Light Curves of the Type II-P Supernova SN 2017eaw: The First 200 Days",
abstract = "We present the results of our UBVRI photometry for the type II-P supernova SN 2017eaw in NGC6946 obtained fromMay 14 to December 7, 2017, at several telescopes, including the 2.5-m telescope at the CaucasusHigh-Altitude Observatory of the SAIMSU. The dates andmagnitudes atmaximumlight and the light-curve parameters have been determined. The color evolution, extinction, and peak luminosity of SN 2017eaw are discussed. The results of our preliminary radiation–gasdynamic simulations of its light curves with the STELLA code describe satisfactorily the UBVRI observational data.",
keywords = "supernovae: SN 2017eaw",
author = "Tsvetkov, {D. Yu} and Shugarov, {S. Yu} and Volkov, {I. M.} and Pavlyuk, {N. N.} and Vozyakova, {O. V.} and Shatsky, {N. I.} and Nikiforova, {A. A.} and Troitsky, {I. S.} and Троицкая, {Юлия Вячеславовна} and Baklanov, {P. V.}",
year = "2018",
month = may,
day = "1",
doi = "10.1134/S1063773718050043",
language = "English",
volume = "44",
pages = "315--323",
journal = "Astronomy Letters",
issn = "1063-7737",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "5",

}

RIS

TY - JOUR

T1 - Light Curves of the Type II-P Supernova SN 2017eaw

T2 - The First 200 Days

AU - Tsvetkov, D. Yu

AU - Shugarov, S. Yu

AU - Volkov, I. M.

AU - Pavlyuk, N. N.

AU - Vozyakova, O. V.

AU - Shatsky, N. I.

AU - Nikiforova, A. A.

AU - Troitsky, I. S.

AU - Троицкая, Юлия Вячеславовна

AU - Baklanov, P. V.

PY - 2018/5/1

Y1 - 2018/5/1

N2 - We present the results of our UBVRI photometry for the type II-P supernova SN 2017eaw in NGC6946 obtained fromMay 14 to December 7, 2017, at several telescopes, including the 2.5-m telescope at the CaucasusHigh-Altitude Observatory of the SAIMSU. The dates andmagnitudes atmaximumlight and the light-curve parameters have been determined. The color evolution, extinction, and peak luminosity of SN 2017eaw are discussed. The results of our preliminary radiation–gasdynamic simulations of its light curves with the STELLA code describe satisfactorily the UBVRI observational data.

AB - We present the results of our UBVRI photometry for the type II-P supernova SN 2017eaw in NGC6946 obtained fromMay 14 to December 7, 2017, at several telescopes, including the 2.5-m telescope at the CaucasusHigh-Altitude Observatory of the SAIMSU. The dates andmagnitudes atmaximumlight and the light-curve parameters have been determined. The color evolution, extinction, and peak luminosity of SN 2017eaw are discussed. The results of our preliminary radiation–gasdynamic simulations of its light curves with the STELLA code describe satisfactorily the UBVRI observational data.

KW - supernovae: SN 2017eaw

UR - http://www.scopus.com/inward/record.url?scp=85047479536&partnerID=8YFLogxK

UR - http://arxiv.org/abs/1801.00340

UR - http://www.mendeley.com/research/light-curves-type-iip-sn-2017eaw-first-200-days

U2 - 10.1134/S1063773718050043

DO - 10.1134/S1063773718050043

M3 - Article

AN - SCOPUS:85047479536

VL - 44

SP - 315

EP - 323

JO - Astronomy Letters

JF - Astronomy Letters

SN - 1063-7737

IS - 5

ER -

ID: 35976170