143:) of the range of massive stars that can produce supernovae. In 2012 he, with two colleagues, explained the fact that often no companion star was found in Type Ia supernovae. Their explanation is that, before the supernova explosion, the companion star of the binary star system evolved into a helium-rich white dwarf, which is difficult to observe. Their explanation solved a problem for the origin of Type I supernovae according to the single degenerate (SD) accretion scenario, in which a red giant or other main sequence star gradually loses mass by accretion onto the nearby white dwarf. In the competing double degenerate (DD) scenario, two white dwarfs with a high carbon-oxygen content merge.
106:
findings indicated that the spectral evolution diversity is not a serious concern in using SNe Ia as cosmological standard candles for determining distances. He was a member of an international team of astronomers that published in 2008 their study using the Subaru
Telescope to observe "light echoes" in the remnant of
324:
Frebel, Anna; Aoki, Wako; Christlieb, Norbert; Ando, Hiroyasu; Asplund, Martin; Barklem, Paul S.; Beers, Timothy C.; Eriksson, Kjell; Fechner, Cora; Fujimoto, Masayuki Y.; Honda, Satoshi; Kajino, Toshitaka; Minezaki, Takeo; Nomoto, Ken'Ichi; Norris, John E.; Ryan, Sean G.; Takada-Hidai, Masahide;
105:
that most core-collapse supernovae are not spherically symmetric but instead elongated in shape. With Maeda and others, he reported that the spectral diversity in Type Ia supernovae (SNe Ia) is a consequence of random directions from which such asymmetric explosions are observed. Their empirical
835:
Maeda, K.; Benetti, S.; Stritzinger, M.; RΓΆpke, F. K.; Folatelli, G.; Sollerman, J.; Taubenberger, S.; Nomoto, K.; Leloudas, G.; Hamuy, M.; Tanaka, M.; Mazzali, P. A.; Elias-Rosa, N. (2010). "An asymmetric explosion as the origin of spectral evolution diversity in type Ia supernovae".
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Thielemann, F.-K.; Brachwitz, F.; Freiburghaus, C.; Kolbe, E.; Martinez-Pinedo, G.; Rauscher, T.; Rembges, F.; Hix, W.R.; LiebendΓΆrfer, M.; Mezzacappa, A.; Kratz, K.-L.; Pfeiffer, B.; Langanke, K.; Nomoto, K.; Rosswog, S.; Schatz, H.; Wiescher, W. (2001). "Element synthesis in stars".
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Mazzali, Paolo A.; Kawabata, Koji S.; Maeda, Keiichi; Nomoto, Ken'Ichi; Filippenko, Alexei V.; Ramirez-Ruiz, Enrico; Benetti, Stefano; Pian, Elena; Deng, Jinsong; Tominaga, Nozomu; Ohyama, Youichi; Iye, Masanori; Foley, Ryan J.; Matheson, Thomas; Wang, Lifan; Gal-Yam, Avishay (2005).
114:'s observation in 1572. The team compared their 2008 observed spectroscopic data with many other supernova spectra to show that Tycho's Supernova is a statistically typical example of a Type Ia supernova. He was part of the research group that revealed that the exceptionally bright
173:
for "lasting contributions to our understanding of the nuclear astrophysics of the universe, including stellar evolution, the synthesis of new elements, the theory of core-collapse and thermonuclear supernovae, and gamma-ray bursts." In 2020 he was awarded the
164:
for showing theoretically that binary systems produce various forms of stellar evolution and can produce "various types of supernovae, hypernovae and gamma-ray bursts, as well as neutron stars and black holes." In 2019 he received the
927:
Krause, Oliver; Tanaka, Masaomi; Usuda, Tomonori; Hattori, Takashi; Goto, Miwa; Birkmann, Stephan; Nomoto, Ken'Ichi (2008). "Tycho Brahe's 1572 supernova as a standard type Ia as revealed by its light-echo spectrum".
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Kawabata, K. S.; Maeda, K.; Nomoto, K.; Taubenberger, S.; Tanaka, M.; Deng, J.; Pian, E.; Hattori, T.; Itagaki, K. (2010). "A massive star origin for an unusual helium-rich supernova in an elliptical galaxy".
59:
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for measuring distances in the
Universe. In 2010, he and colleagues succeeded in detecting a supernova (SN 2005cz), which is a core-collapse supernova with progenitor star at the low-mass end (
441:
Iwamoto, Nobuyuki; Umeda, Hideyuki; Tominaga, Nozomu; Nomoto, Ken'Ichi; Maeda, Keiichi (2005). "The First
Chemical Enrichment in the Universe and the Formation of Hyper Metal-Poor Stars".
58:
he was an assistant professor from 1976 to 1981. At the
University of Tokyo he became an assistant professor in 1982, an associate professor in 1985, and a full professor in 1993. At the
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66:) he was a principal investigator from 2007 to 2017, as well as a project professor from 2008 to 2017, and is since 2017 a visiting senior scientist. He was a research associate at
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Hachisu, Izumi; Kato, Mariko; Nomoto, Ken'Ichi (2012). "Final Fates of
Rotating White Dwarfs and Their Companions in the Single Degenerate Model of Type Ia Supernovae".
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Heger, A.; Nomoto, K.; Leung, S-C; Tolstov, A.; Wongwathanarat, A.; Gessner, A.; Gabler, M.; Ertl, T.; Melson, T.; Kresse, D.; Janka, H-T; Stockinger, G. (2020).
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Bennett, M. E.; Hirschi, R.; Pignatari, M.; Diehl, S.; Fryer, C.; Herwig, F.; Hungerford, A.; Nomoto, K.; Rockefeller, G.; Timmes, F. X.; Wiescher, M. (2012).
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Nomoto, Ken'Ichi; Kobayashi, Chiaki; Tominaga, Nozomu (2013). "Nucleosynthesis in Stars and the
Chemical Enrichment of Galaxies".
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Ferrand, Gilles; Tanikawa, Ataru; Warren, Donald C.; Nagataki, Shigehiro; Safi-Harb, Samar; Decourchelle, Anne (2022).
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98:. He is now the University of Tokyo's Hamamatsu Professor in the endowed research unit, Dark Side of the Universe.
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1223:"The Double Detonation of a Double-degenerate System, from Type Ia Supernova Explosion to its Supernova Remnant"
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Rayet, M.; Arnould, M.; Hashimoto, M.; Prantzos, N.; Nomoto, K. (1995). "The p-process in Type II supernovae".
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677:"Three-dimensional models of core-collapse supernovae from low-mass progenitors with implications for Crab"
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596:"Evidence for Type Ia supernovae diversity from ultraviolet observations with the Hubble Space Telescope"
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110:; such light echoes bounced off dust particle surrounding the remnant and reached Earth 436 years after
26:, born 1 December 1946 in Tokyo) is a Japanese astrophysicist and astronomer, known for his research on
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Nomoto Group, Kavli
Institute for the Physics and Mathematics of the Universe, the University of Tokyo
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due to its fast rotation. The discovery has implications for the common use of Type Ia supernovae as
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1165:"Rapidly rotating white dwarf stars can solve the missing companion problem for Type Ia supernovae"
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543:"The effect of 12C +12C rate uncertainties on the evolution and nucleosynthesis of massive stars"
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Tsangarides, Stelios; Yoshii, Yuzuru (2005). "Nucleosynthetic signatures of the first stars".
223:"Accreting white dwarf models for CAL 83, CAL 87 and other ultrasoft X-ray sources in the LMC"
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384:"An Asymmetric Energetic Type Ic Supernova Viewed Off-Axis, and a Link to Gamma Ray Bursts"
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In 2008 he, with his colleagues
Keiichi Maeda and Masaomi Tanaka, discovered by using the
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1281:"Kavli IPMU Senior Scientist Ken'ichi Nomoto awarded the Order of the Sacred Treasure"
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1020:"A Massive Star Origin for An Unusual Helium-Rich Supernovae in An Elliptical Galaxy"
806:"Strengthening the case for the dark energy! Type Ia supernova are after all uniform"
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van den Heuvel, E.P.J.; Bhattacharya, D.; Nomoto, K.; Rappaport, S.A. (August 1992).
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898:"Subaru sees Tycho's New Star via Echo Light: K.Nomoto and His International Team"
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with a BS in 1969 and a PhD in 1974. As a postdoc he was a research fellow of the
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74:(1979β1981) and has held visiting positions at several institutions, including
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1314:"INT 14-2a: Ken'ichi Nomoto, Progenitors of neutron star forming supernovae"
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Kavli
Institute for the Physics and Mathematics of the Universe (IPMU)
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Advanced
Statistical Methods for Astrophysical Probes of Cosmology
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788:"Supernovae are NOT round: Spectroscopy by the Subaru Telescope"
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Kavli Institute for the Physics and Mathematics of the Universe
1326:"Public Lecture of Kenichi Nomoto at MG14 β Rome, July 2015"
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Press Releases, School of Science, the University of Tokyo
190:"Formation of dust grains in the ejecta of SN 1987A. II"
188:
Kozasa, T.; Hasegawa, H.; Nomoto, K. (September 1991).
752:"2019 Hans A. Bethe Prize Recipient, Ken'ichi Nomoto"
1344:. NTU β Institute of Advanced Studies. 19 June 2018.
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729:"Ken'ichi Nomoto Wins 2015 Marcel Grossman Award"
681:Monthly Notices of the Royal Astronomical Society
547:Monthly Notices of the Royal Astronomical Society
502:Monthly Notices of the Royal Astronomical Society
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1627:Recipients of the Order of the Sacred Treasure
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647:Annual Review of Astronomy and Astrophysics
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1338:"Transient Universe 03 01 Ken'ichi Nomoto"
1194:March, Marisa Cristina (13 January 2013).
498:"The broad-lined Type Ic supernova 2003jd"
52:Japan Society for the Promotion of Science
1607:Academic staff of the University of Tokyo
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278:Progress in Particle and Nuclear Physics
118:had a progenitor star with a mass (1.44
1346:(Conference on The Transient Universe,
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96:Kavli Institute for Theoretical Physics
84:University of Illinois Urbana-Champaign
46:Nomoto graduated in astronomy from the
16:Japanese astrophysicist and astronomer
990:"The Most Luminous Type Ia Supernova"
80:Max Planck Institute for Astrophysics
7:
594:Wang, Xiaofeng; et al. (2012).
667:10.1146/annurev-astro-082812-140956
1320:. INT UW Seattle. 6 November 2014.
1171:. 4 September 2012. Archived from
14:
1617:21st-century Japanese astronomers
1612:20th-century Japanese astronomers
904:. 1 December 2008. Archived from
496:Valenti, S.; et al. (2007).
157:Institut d'Astrophysique de Paris
116:Type Ia supernova named SN 2009dc
1348:Nanyang Technological University
578:10.1111/j.1365-2966.2012.20193.x
525:10.1111/j.1365-2966.2007.12647.x
154:, and in 2010 a medal from the
1350:, 26 February to 1 March 2018)
88:Brookhaven National Laboratory
1:
1026:. 20 May 2010. Archived from
812:. 1 July 2010. Archived from
308:10.1016/S0146-6410(01)00103-X
1200:. Springer. pp. 46β49.
176:Order of the Sacred Treasure
146:Nomoto received in 1989 the
630:10.1088/0004-637X/749/2/126
108:Tycho's Supernova (SN 1572)
72:Goddard Space Flight Center
1643:
1602:University of Tokyo alumni
1143:10.1088/2041-8205/756/1/L4
256:Astronomy and Astrophysics
227:Astronomy and Astrophysics
194:Astronomy and Astrophysics
160:. In 2015 he received the
1332:. ICRANet. 16 March 2016.
1227:The Astrophysical Journal
1113:The Astrophysical Journal
756:American Physical Society
600:The Astrophysical Journal
171:American Physical Society
1622:Japanese astrophysicists
1258:10.3847/1538-4357/ac5c58
36:origin of heavy elements
1461:Friedrich K. Thielemann
659:2013ARA&A..51..457N
473:10.1126/science.1112997
418:10.1126/science.1111384
268:1995A&A...298..517R
239:1992A&A...262...97V
206:1991A&A...249..474K
92:University of Amsterdam
1500:Silvia Torres-Peimbert
1490:Christopher J. Pethick
1449:Alastair G. W. Cameron
1431:Michael C. F. Wiescher
996:. 2009. Archived from
704:10.1093/mnras/staa1691
162:Marcel Grossmann Award
148:Nishina Memorial Prize
1407:Edwin Ernest Salpeter
182:Selected publications
127:) slightly above the
82:(1982 and 1983), the
671:(over 700 citations)
377:(over 700 citations)
42:Education and career
1401:John Norris Bahcall
1385:Hans A. Bethe Prize
1249:2022ApJ...930...92F
1135:2012ApJ...756L...4H
1082:10.1038/nature09055
1074:2010Natur.465..326K
1030:on 11 February 2021
960:10.1038/nature07608
952:2008Natur.456..617K
868:10.1038/nature09122
860:2010Natur.466...82M
622:2012ApJ...749..126W
569:2012MNRAS.420.3047B
465:2005Sci...309..451I
410:2005Sci...308.1284M
394:(5726): 1284β1287.
357:10.1038/nature03455
349:2005Natur.434..871F
300:2001PrPNP..46....5T
167:Hans A. Bethe Prize
152:Japan Academy Medal
129:Chandrasekhar limit
48:University of Tokyo
1536:Keith Alison Olive
1524:Vassiliki Kalogera
816:on 18 October 2021
794:. 31 January 2008.
56:Ibaraki University
1579:
1578:
1530:Stuart L. Shapiro
1512:Karl Ludwig Kratz
1302:"Ken'ichi Nomoto"
1175:on 6 October 2022
1058:(7296): 326β328.
936:(7222): 617β619.
770:"Ken'ichi Nomoto"
449:(5733): 451β453.
333:(7035): 871β873.
90:(1985β1986), the
28:stellar evolution
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1506:George M. Fuller
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1419:Gerald E. Brown
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