SN 2020pvb: A Type IIn-P supernova with a precursor outburst

N. Elias-Rosa; S. J. Brennan; S. Benetti; E. Cappellaro; A. Pastorello; A. Kozyreva; P. Lundqvist; M. Fraser; J. P. Anderson; Y. Z. Cai; T. W. Chen; M. Dennefeld; M. Gromadzki; C. P. Gutiérrez; N. Ihanec; C. Inserra; E. Kankare; R. Kotak; S. Mattila; S. Moran; T. E. Müller-Bravo; P. J. Pessi; G. Pignata; A. Reguitti; T. M. Reynolds; S. J. Smartt; K. Smith; L. Tartaglia; G. Valerin; T. De Boer; K. Chambers; A. Gal-Yam; H. Gao; S. Geier; P. A. Mazzali; M. Nicholl; F. Ragosta; A. Rest; O. Yaron; D. R. Young

doi:10.1051/0004-6361/202348790

SN 2020pvb: A Type IIn-P supernova with a precursor outburst

N. Elias-Rosa, S. J. Brennan, S. Benetti, E. Cappellaro, A. Pastorello, A. Kozyreva, P. Lundqvist, M. Fraser, J. P. Anderson, Y. Z. Cai, T. W. Chen, M. Dennefeld, M. Gromadzki, C. P. Gutiérrez, N. Ihanec, C. Inserra, E. Kankare, R. Kotak, S. Mattila, S. MoranT. E. Müller-Bravo, P. J. Pessi, G. Pignata, A. Reguitti, T. M. Reynolds, S. J. Smartt, K. Smith, L. Tartaglia, G. Valerin, T. De Boer, K. Chambers, A. Gal-Yam, H. Gao, S. Geier, P. A. Mazzali, M. Nicholl, F. Ragosta, A. Rest, O. Yaron, D. R. Young

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摘要

We present photometric and spectroscopic datasets for SN 2020pvb, a Type IIn-P supernova (SN) that is similar to SNe 1994W, 2005cl, 2009kn, and 2011ht, with a precursor outburst detected (PS1 w band ∼- 13.8 mag) around four months before the B-band maximum light. SN 2020pvb presents a relatively bright light curve that peaked at M_B = -17.95 ± 0.30 mag and a plateau that lasted at least 40 days before going into solar conjunction. After this, the object was no longer visible at phases > 150 days above - 12.5 mag in the B band, suggesting that the SN 2020pvb ejecta interact with a dense, spatially confined circumstellar envelope. SN 2020pvb shows strong Balmer lines and a forest of Fe II lines with narrow P Cygni profiles in its spectra. Using archival images from the Hubble Space Telescope, we constrained the progenitor of SN 2020pvb to have a luminosity of log(L/L_⊙)≤5.4, ruling out any single star progenitor over 50 M_⊙. SN 2020pvb is a Type IIn-P whose progenitor star had an outburst*sim;0.5 yr before the final explosion; the material lost during this outburst probably plays a role in shaping the physical properties of the SN.

原文	???core.languages.en_GB???
文章編號	A13
期刊	Astronomy and Astrophysics
卷	686
DOIs	https://doi.org/10.1051/0004-6361/202348790
出版狀態	已出版 - 1 6月 2024

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Elias-Rosa, N., Brennan, S. J., Benetti, S., Cappellaro, E., Pastorello, A., Kozyreva, A., Lundqvist, P., Fraser, M., Anderson, J. P., Cai, Y. Z., Chen, T. W., Dennefeld, M., Gromadzki, M., Gutiérrez, C. P., Ihanec, N., Inserra, C., Kankare, E., Kotak, R., Mattila, S., ... Young, D. R. (2024). SN 2020pvb: A Type IIn-P supernova with a precursor outburst. Astronomy and Astrophysics, 686, 文章 A13. https://doi.org/10.1051/0004-6361/202348790

@article{1e4aa71752c149f2bf3e4f3fb59a75ff,

title = "SN 2020pvb: A Type IIn-P supernova with a precursor outburst",

abstract = "We present photometric and spectroscopic datasets for SN 2020pvb, a Type IIn-P supernova (SN) that is similar to SNe 1994W, 2005cl, 2009kn, and 2011ht, with a precursor outburst detected (PS1 w band ∼- 13.8 mag) around four months before the B-band maximum light. SN 2020pvb presents a relatively bright light curve that peaked at MB = -17.95 ± 0.30 mag and a plateau that lasted at least 40 days before going into solar conjunction. After this, the object was no longer visible at phases > 150 days above - 12.5 mag in the B band, suggesting that the SN 2020pvb ejecta interact with a dense, spatially confined circumstellar envelope. SN 2020pvb shows strong Balmer lines and a forest of Fe II lines with narrow P Cygni profiles in its spectra. Using archival images from the Hubble Space Telescope, we constrained the progenitor of SN 2020pvb to have a luminosity of log(L/L⊙)≤5.4, ruling out any single star progenitor over 50 M⊙. SN 2020pvb is a Type IIn-P whose progenitor star had an outburst*sim;0.5 yr before the final explosion; the material lost during this outburst probably plays a role in shaping the physical properties of the SN.",

keywords = "Supernovae: general, Supernovae: individual: SN 2020pvb",

author = "N. Elias-Rosa and Brennan, {S. J.} and S. Benetti and E. Cappellaro and A. Pastorello and A. Kozyreva and P. Lundqvist and M. Fraser and Anderson, {J. P.} and Cai, {Y. Z.} and Chen, {T. W.} and M. Dennefeld and M. Gromadzki and Guti{\'e}rrez, {C. P.} and N. Ihanec and C. Inserra and E. Kankare and R. Kotak and S. Mattila and S. Moran and M{\"u}ller-Bravo, {T. E.} and Pessi, {P. J.} and G. Pignata and A. Reguitti and Reynolds, {T. M.} and Smartt, {S. J.} and K. Smith and L. Tartaglia and G. Valerin and {De Boer}, T. and K. Chambers and A. Gal-Yam and H. Gao and S. Geier and Mazzali, {P. A.} and M. Nicholl and F. Ragosta and A. Rest and O. Yaron and Young, {D. R.}",

note = "Publisher Copyright: {\textcopyright} The Authors 2024.",

year = "2024",

month = jun,

day = "1",

doi = "10.1051/0004-6361/202348790",

language = "???core.languages.en_GB???",

volume = "686",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

}

Elias-Rosa, N, Brennan, SJ, Benetti, S, Cappellaro, E, Pastorello, A, Kozyreva, A, Lundqvist, P, Fraser, M, Anderson, JP, Cai, YZ, Chen, TW, Dennefeld, M, Gromadzki, M, Gutiérrez, CP, Ihanec, N, Inserra, C, Kankare, E, Kotak, R, Mattila, S, Moran, S, Müller-Bravo, TE, Pessi, PJ, Pignata, G, Reguitti, A, Reynolds, TM, Smartt, SJ, Smith, K, Tartaglia, L, Valerin, G, De Boer, T, Chambers, K, Gal-Yam, A, Gao, H, Geier, S, Mazzali, PA, Nicholl, M, Ragosta, F, Rest, A, Yaron, O & Young, DR 2024, 'SN 2020pvb: A Type IIn-P supernova with a precursor outburst', Astronomy and Astrophysics, 卷 686, A13. https://doi.org/10.1051/0004-6361/202348790

TY - JOUR

T1 - SN 2020pvb

T2 - A Type IIn-P supernova with a precursor outburst

AU - Elias-Rosa, N.

AU - Brennan, S. J.

AU - Benetti, S.

AU - Cappellaro, E.

AU - Pastorello, A.

AU - Kozyreva, A.

AU - Lundqvist, P.

AU - Fraser, M.

AU - Anderson, J. P.

AU - Cai, Y. Z.

AU - Chen, T. W.

AU - Dennefeld, M.

AU - Gromadzki, M.

AU - Gutiérrez, C. P.

AU - Ihanec, N.

AU - Inserra, C.

AU - Kankare, E.

AU - Kotak, R.

AU - Mattila, S.

AU - Moran, S.

AU - Müller-Bravo, T. E.

AU - Pessi, P. J.

AU - Pignata, G.

AU - Reguitti, A.

AU - Reynolds, T. M.

AU - Smartt, S. J.

AU - Smith, K.

AU - Tartaglia, L.

AU - Valerin, G.

AU - De Boer, T.

AU - Chambers, K.

AU - Gal-Yam, A.

AU - Gao, H.

AU - Geier, S.

AU - Mazzali, P. A.

AU - Nicholl, M.

AU - Ragosta, F.

AU - Rest, A.

AU - Yaron, O.

AU - Young, D. R.

PY - 2024/6/1

Y1 - 2024/6/1

N2 - We present photometric and spectroscopic datasets for SN 2020pvb, a Type IIn-P supernova (SN) that is similar to SNe 1994W, 2005cl, 2009kn, and 2011ht, with a precursor outburst detected (PS1 w band ∼- 13.8 mag) around four months before the B-band maximum light. SN 2020pvb presents a relatively bright light curve that peaked at MB = -17.95 ± 0.30 mag and a plateau that lasted at least 40 days before going into solar conjunction. After this, the object was no longer visible at phases > 150 days above - 12.5 mag in the B band, suggesting that the SN 2020pvb ejecta interact with a dense, spatially confined circumstellar envelope. SN 2020pvb shows strong Balmer lines and a forest of Fe II lines with narrow P Cygni profiles in its spectra. Using archival images from the Hubble Space Telescope, we constrained the progenitor of SN 2020pvb to have a luminosity of log(L/L⊙)≤5.4, ruling out any single star progenitor over 50 M⊙. SN 2020pvb is a Type IIn-P whose progenitor star had an outburst*sim;0.5 yr before the final explosion; the material lost during this outburst probably plays a role in shaping the physical properties of the SN.

AB - We present photometric and spectroscopic datasets for SN 2020pvb, a Type IIn-P supernova (SN) that is similar to SNe 1994W, 2005cl, 2009kn, and 2011ht, with a precursor outburst detected (PS1 w band ∼- 13.8 mag) around four months before the B-band maximum light. SN 2020pvb presents a relatively bright light curve that peaked at MB = -17.95 ± 0.30 mag and a plateau that lasted at least 40 days before going into solar conjunction. After this, the object was no longer visible at phases > 150 days above - 12.5 mag in the B band, suggesting that the SN 2020pvb ejecta interact with a dense, spatially confined circumstellar envelope. SN 2020pvb shows strong Balmer lines and a forest of Fe II lines with narrow P Cygni profiles in its spectra. Using archival images from the Hubble Space Telescope, we constrained the progenitor of SN 2020pvb to have a luminosity of log(L/L⊙)≤5.4, ruling out any single star progenitor over 50 M⊙. SN 2020pvb is a Type IIn-P whose progenitor star had an outburst*sim;0.5 yr before the final explosion; the material lost during this outburst probably plays a role in shaping the physical properties of the SN.

KW - Supernovae: general

KW - Supernovae: individual: SN 2020pvb

UR - http://www.scopus.com/inward/record.url?scp=85194376112&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/202348790

DO - 10.1051/0004-6361/202348790

M3 - 期刊論文

AN - SCOPUS:85194376112

SN - 0004-6361

VL - 686

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A13

ER -

SN 2020pvb: A Type IIn-P supernova with a precursor outburst

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