The late-time light curve of the type la supernova 2000cx

被引：0

作者：

Sollerman, J. ^{[1
]}

Lindahl, J. ^{[1
,2
]}

Kozma, C. ^{[1
]}

Challis, P. ^{[3
]}

Filippenko, A.V. ^{[4
]}

Fransson, C. ^{[1
]}

Garnavich, P.M. ^{[5
]}

Leibundgut, B. ^{[6
]}

Li, W. ^{[4
]}

Lundqvist, P. ^{[1
]}

Milne, P. ^{[7
]}

Spyromilio, J. ^{[6
]}

Kirshner, R.P. ^{[3
]}

机构：

[1] Stockholm Observatory, AlbaNova, Department of Astronomy, 106 91 Stockholm, Sweden

[2] Onsala Space Observatory, Chalmers University of Technology, 439 92 Onsala, Sweden

[3] Harvard-Smithsonian Ctr. Astrophys., 60 Garden Street, Cambridge, MA 02138, United States

[4] Department of Astronomy, University of California, Berkeley, CA 94720-3411, United States

[5] Physics Department, University of Notre Dame, Notre Dame, IN 46566, United States

[6] European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany

[7] Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, United States

来源：

Astronomy and Astrophysics | 1600年 / 428卷 / 02期

关键词：

Number: -, Acronym: NSF, Sponsor: National Science Foundation, Number: 0307894,9987438, Acronym: MPS, Sponsor: Directorate for Mathematical and Physical Sciences, Number: -, Acronym: MPS, Sponsor: Directorate for Mathematical and Physical Sciences,;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

引用

页码：555 / 568

共 50 条

[41] A comparative study of late-time light curves of Type Ic Super-novae
Misra, Kuntal
Fruchter, Andrew S.
PROCEEDINGS OF THE 31ST MEETING OF THE ASTRONOMICAL SOCIETY OF INDIA, 2013, 2013, : 88 - 88
[42] LATE-TIME LIGHT CURVES OF TYPE II SUPERNOVAE: PHYSICAL PROPERTIES OF SUPERNOVAE AND THEIR ENVIRONMENT
Otsuka, Masaaki
Meixner, Margaret
Panagia, Nino
Fabbri, Joanna
Barlow, Michael J.
Clayton, Geoffrey C.
Gallagher, Joseph S.
Sugerman, Ben E. K.
Wesson, Roger
Andrews, Jennifer E.
Ercolano, Barbara
Welch, Douglas
ASTROPHYSICAL JOURNAL, 2012, 744 (01):
[43] Diffuse supernova neutrino background as a probe of late-time neutrino mass generation
de Gouvea, Andre
Martinez-Soler, Ivan
Perez-Gonzalez, Yuber F.
Sen, Manibrata
PHYSICAL REVIEW D, 2022, 106 (10)
[44] Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties
Maguire, K.
Sim, S. A.
Shingles, L.
Spyromilio, J.
Jerkstrand, A.
Sullivan, M.
Chen, T. -W.
Cartier, R.
Dimitriadis, G.
Frohmaier, C.
Galbany, L.
Gutierrez, C. P.
Hosseinzadeh, G.
Howell, D. A.
Inserra, C.
Rudy, R.
Sollerman, J.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 477 (03) : 3567 - 3582
[45] LATE-TIME SOURCE OF ATOMIC LIGHT IN HELIUM AFTERGLOW
HURT, WB
COLLINS, CB
BULLETIN OF THE AMERICAN PHYSICAL SOCIETY, 1969, 14 (02): : 257 - &
[46] The progenitor mass of the Type IIP supernova SN 2004et from late-time spectral modeling
Jerkstrand, A.
Fransson, C.
Maguire, K.
Smartt, S.
Ergon, M.
Spyromilio, J.
ASTRONOMY & ASTROPHYSICS, 2012, 546
[47] Detailed analysis of early to late-time spectra of supernova 1993J
Matheson, T
Filippenko, AV
Ho, LC
Barth, AJ
Leonard, DC
ASTRONOMICAL JOURNAL, 2000, 120 (03): : 1499 - 1515
[48] THEORETICAL LIGHT-CURVE OF A TYPE IIP SUPERNOVA
EASTMAN, RG
WOOSLEY, SE
WEAVER, TA
PINTO, PA
ASTROPHYSICAL JOURNAL, 1994, 430 (01): : 300 - 310
[49] HYPOTHESIS FOR TYPE-I SUPERNOVA LIGHT CURVE
LEVENTHAL, M
MCCALL, SL
NATURE, 1975, 255 (5511) : 690 - 692
[50] LATE-TIME SOURCE OF ATOMIC LIGHT IN HELIUM AFTERGLOW
COLLINS, CB
HURT, WB
PHYSICAL REVIEW, 1969, 177 (01): : 257 - &

← 1 2 3 4 5 →