The delay of shock breakout due to circumstellar material evident in most type II supernovae

F. Forster; T. J. Moriya; J. C. Maureira; J. P. Anderson; S. Blinnikov; F. Bufano; G. Cabrera-Vives; A. Clocchiatti; T. de Jaeger; P. A. Estevez; L. Galbany; S. Gonzalez-Gaitan; G. Graefener; M. Hamuy; E. Y. Hsiao; P. Huentelemu; P. Huijse; H. Kuncarayakti; J. Martinez; G. Medina; F. Olivares E; G. Pignata; A. Razza; R. De Los Reyes; J. San Martin; R. C. Smith; E. Vera; A. K. Vivas; A. de Ugarte Postigo; S-C Yoon; C. Ashall; M. Fraser; A. Gal-Yam; E. Kankare; L. Le Guillou; P. A. Mazzali; N. A. Walton; D. R. Young

doi:10.1038/s41550-018-0563-4

The delay of shock breakout due to circumstellar material evident in most type II supernovae

F. Forster, T. J. Moriya, J. C. Maureira, J. P. Anderson, S. Blinnikov, F. Bufano, G. Cabrera-Vives, A. Clocchiatti, T. de Jaeger, P. A. Estevez, L. Galbany, S. Gonzalez-Gaitan, G. Graefener, M. Hamuy, E. Y. Hsiao, P. Huentelemu, P. Huijse, H. Kuncarayakti, J. Martinez, G. MedinaF. Olivares E, G. Pignata, A. Razza, R. De Los Reyes, J. San Martin, R. C. Smith, E. Vera, A. K. Vivas, A. de Ugarte Postigo, S-C Yoon, C. Ashall, M. Fraser, A. Gal-Yam, E. Kankare, L. Le Guillou, P. A. Mazzali, N. A. Walton, D. R. Young

Department of Particle Physics and Astrophysics

Weizmann Institute of Science

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

Abstract

Type II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout (SBO), a short-lived phenomenon that can last for hours to days depending on the density at shock emergence. We present 26 rising optical light curves of SN II candidates discovered shortly after explosion by the High Cadence Transient Survey and derive physical parameters based on hydrodynamical models using a Bayesian approach. We observe a steep rise of a few days in 24 out of 26 SN II candidates, indicating the systematic detection of SBOs in a dense circumstellar matter consistent with a mass loss rate of Ṁ> 10 ⁻⁴M _⊙ yr ⁻¹ or a dense atmosphere. This implies that the characteristic hour-timescale signature of stellar envelope SBOs may be rare in nature and could be delayed into longer-lived circumstellar material SBOs in most SNe II.

Original language	English
Pages (from-to)	808-818
Number of pages	11
Journal	Nature Astronomy
Volume	2
Early online date	3 Sep 2018
DOIs	https://doi.org/10.1038/s41550-018-0563-4
State	Published - Oct 2018

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics

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http://researchonline.ljmu.ac.uk/id/eprint/11045/1/The%20delay%20of%20shock%20breakout%20due%20to%20circumstellar%20material%20evident%20in%20most%20type%20II%20supernovae.pdfLicense: Unspecified

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Forster, F., Moriya, T. J., Maureira, J. C., Anderson, J. P., Blinnikov, S., Bufano, F., Cabrera-Vives, G., Clocchiatti, A., de Jaeger, T., Estevez, P. A., Galbany, L., Gonzalez-Gaitan, S., Graefener, G., Hamuy, M., Hsiao, E. Y., Huentelemu, P., Huijse, P., Kuncarayakti, H., Martinez, J., ... Young, D. R. (2018). The delay of shock breakout due to circumstellar material evident in most type II supernovae. Nature Astronomy, 2, 808-818. https://doi.org/10.1038/s41550-018-0563-4

@article{2353cc32c857450a977936708b433cb4,

title = "The delay of shock breakout due to circumstellar material evident in most type II supernovae",

abstract = "Type II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout (SBO), a short-lived phenomenon that can last for hours to days depending on the density at shock emergence. We present 26 rising optical light curves of SN II candidates discovered shortly after explosion by the High Cadence Transient Survey and derive physical parameters based on hydrodynamical models using a Bayesian approach. We observe a steep rise of a few days in 24 out of 26 SN II candidates, indicating the systematic detection of SBOs in a dense circumstellar matter consistent with a mass loss rate of Ṁ> 10 −4M ⊙ yr −1 or a dense atmosphere. This implies that the characteristic hour-timescale signature of stellar envelope SBOs may be rare in nature and could be delayed into longer-lived circumstellar material SBOs in most SNe II. ",

author = "F. Forster and Moriya, {T. J.} and Maureira, {J. C.} and Anderson, {J. P.} and S. Blinnikov and F. Bufano and G. Cabrera-Vives and A. Clocchiatti and {de Jaeger}, T. and Estevez, {P. A.} and L. Galbany and S. Gonzalez-Gaitan and G. Graefener and M. Hamuy and Hsiao, {E. Y.} and P. Huentelemu and P. Huijse and H. Kuncarayakti and J. Martinez and G. Medina and {Olivares E}, F. and G. Pignata and A. Razza and Reyes, {R. De Los} and {San Martin}, J. and Smith, {R. C.} and E. Vera and Vivas, {A. K.} and {de Ugarte Postigo}, A. and S-C Yoon and C. Ashall and M. Fraser and A. Gal-Yam and E. Kankare and {Le Guillou}, L. and Mazzali, {P. A.} and Walton, {N. A.} and Young, {D. R.}",

year = "2018",

month = oct,

doi = "10.1038/s41550-018-0563-4",

language = "الإنجليزيّة",

volume = "2",

pages = "808--818",

journal = "Nature Astronomy",

issn = "2397-3366",

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Forster, F, Moriya, TJ, Maureira, JC, Anderson, JP, Blinnikov, S, Bufano, F, Cabrera-Vives, G, Clocchiatti, A, de Jaeger, T, Estevez, PA, Galbany, L, Gonzalez-Gaitan, S, Graefener, G, Hamuy, M, Hsiao, EY, Huentelemu, P, Huijse, P, Kuncarayakti, H, Martinez, J, Medina, G, Olivares E, F, Pignata, G, Razza, A, Reyes, RDL, San Martin, J, Smith, RC, Vera, E, Vivas, AK, de Ugarte Postigo, A, Yoon, S-C, Ashall, C, Fraser, M, Gal-Yam, A, Kankare, E, Le Guillou, L, Mazzali, PA, Walton, NA & Young, DR 2018, 'The delay of shock breakout due to circumstellar material evident in most type II supernovae', Nature Astronomy, vol. 2, pp. 808-818. https://doi.org/10.1038/s41550-018-0563-4

TY - JOUR

T1 - The delay of shock breakout due to circumstellar material evident in most type II supernovae

AU - Forster, F.

AU - Moriya, T. J.

AU - Maureira, J. C.

AU - Anderson, J. P.

AU - Blinnikov, S.

AU - Bufano, F.

AU - Cabrera-Vives, G.

AU - Clocchiatti, A.

AU - de Jaeger, T.

AU - Estevez, P. A.

AU - Galbany, L.

AU - Gonzalez-Gaitan, S.

AU - Graefener, G.

AU - Hamuy, M.

AU - Hsiao, E. Y.

AU - Huentelemu, P.

AU - Huijse, P.

AU - Kuncarayakti, H.

AU - Martinez, J.

AU - Medina, G.

AU - Olivares E, F.

AU - Pignata, G.

AU - Razza, A.

AU - Reyes, R. De Los

AU - San Martin, J.

AU - Smith, R. C.

AU - Vera, E.

AU - Vivas, A. K.

AU - de Ugarte Postigo, A.

AU - Yoon, S-C

AU - Ashall, C.

AU - Fraser, M.

AU - Gal-Yam, A.

AU - Kankare, E.

AU - Le Guillou, L.

AU - Mazzali, P. A.

AU - Walton, N. A.

AU - Young, D. R.

PY - 2018/10

Y1 - 2018/10

N2 - Type II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout (SBO), a short-lived phenomenon that can last for hours to days depending on the density at shock emergence. We present 26 rising optical light curves of SN II candidates discovered shortly after explosion by the High Cadence Transient Survey and derive physical parameters based on hydrodynamical models using a Bayesian approach. We observe a steep rise of a few days in 24 out of 26 SN II candidates, indicating the systematic detection of SBOs in a dense circumstellar matter consistent with a mass loss rate of Ṁ> 10 −4M ⊙ yr −1 or a dense atmosphere. This implies that the characteristic hour-timescale signature of stellar envelope SBOs may be rare in nature and could be delayed into longer-lived circumstellar material SBOs in most SNe II.

AB - Type II supernovae (SNe II) originate from the explosion of hydrogen-rich supergiant massive stars. Their first electromagnetic signature is the shock breakout (SBO), a short-lived phenomenon that can last for hours to days depending on the density at shock emergence. We present 26 rising optical light curves of SN II candidates discovered shortly after explosion by the High Cadence Transient Survey and derive physical parameters based on hydrodynamical models using a Bayesian approach. We observe a steep rise of a few days in 24 out of 26 SN II candidates, indicating the systematic detection of SBOs in a dense circumstellar matter consistent with a mass loss rate of Ṁ> 10 −4M ⊙ yr −1 or a dense atmosphere. This implies that the characteristic hour-timescale signature of stellar envelope SBOs may be rare in nature and could be delayed into longer-lived circumstellar material SBOs in most SNe II.

UR - http://www.scopus.com/inward/record.url?scp=85058706062&partnerID=8YFLogxK

U2 - 10.1038/s41550-018-0563-4

DO - 10.1038/s41550-018-0563-4

M3 - مقالة

SN - 2397-3366

VL - 2

SP - 808

EP - 818

JO - Nature Astronomy

JF - Nature Astronomy

ER -

The delay of shock breakout due to circumstellar material evident in most type II supernovae

Abstract

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