CNO cycle (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "CNO cycle" in English language version.

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12doi.org

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10harvard.edu

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4arxiv.org

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4nih.gov

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4semanticscholar.org

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2archive.org

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2books.google.com

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2worldcat.org

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2web.archive.org

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1nature.com

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1phys.org

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1caltech.edu

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1aps.org

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1iop.org

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1handle.net

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aps.org (Global: 1,503^rd place; English: 1,378^th place)

physics.aps.org

Bardi, Jason Socrates (23 January 2008). "Landmarks: What makes the stars shine?". Physical Review Focus. Vol. 21, no. 3. doi:10.1103/physrevfocus.21.3. Retrieved 26 November 2018.

archive.org (Global: 6^th place; English: 6^th place)

Salaris, Maurizio; Cassisi, Santi (2005). Evolution of Stars and Stellar Populations. John Wiley and Sons. pp. 119–121. ISBN 0-470-09220-3.
Krane, Kenneth S. (1988). Introductory Nuclear Physics. John Wiley & Sons. p. 537. ISBN 0-471-80553-X.

arxiv.org (Global: 69^th place; English: 59^th place)

Agostini, M.; Altenmüller, K.; et al. (The BOREXINO collaboration) (25 June 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. PMID 33239797. S2CID 227174644.
Schuler, S.C.; King, J.R.; The, L.-S. (2009). "Stellar Nucleosynthesis in the Hyades open cluster". The Astrophysical Journal. 701 (1): 837–849. arXiv:0906.4812. Bibcode:2009ApJ...701..837S. doi:10.1088/0004-637X/701/1/837. S2CID 10626836.
Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;
Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P.; et al. (LUNA Collaboration) (2006). "First measurement of the ¹⁴N(p,γ)¹⁵O cross section down to 70 keV". Physics Letters B. 634 (5–6): 483–487. arXiv:nucl-ex/0602012. Bibcode:2006PhLB..634..483L. doi:10.1016/j.physletb.2006.02.021. S2CID 16875233.

books.google.com (Global: 3^rd place; English: 3^rd place)

Reid, I. Neill; Hawley, Suzanne L. (2005). "The structure, formation, and evolution of low-mass stars and brown dwarfs – Energy generation". New Light on Dark Stars: Red dwarfs, low-mass stars, brown dwarfs. Springer-Praxis Books in Astrophysics and Astronomy (2nd ed.). Springer Science & Business Media. pp. 108–111. ISBN 3-540-25124-3.
Ray, Alak (2010). "Massive stars as thermonuclear reactors and their explosions following core collapse". In Goswami, Aruna; Reddy, B. Eswar (eds.). Principles and Perspectives in Cosmochemistry. Springer Science & Business Media. p. 233. ISBN 978-3-642-10368-1.

caltech.edu (Global: 887^th place; English: 714^th place)

authors.library.caltech.edu

Bethe, Hans A.; Bacher, Robert (1936). "Nuclear Physics, A: Stationary states of nuclei" (PDF). Reviews of Modern Physics. 8 (2): 82–229. Bibcode:1936RvMP....8...82B. doi:10.1103/RevModPhys.8.82.

core.ac.uk (Global: 1,734^th place; English: 1,312^th place)

Depalo, Rosanna. "The neon-sodium cycle: Study of the 22Ne(p, γ)23Na reaction at astrophysical energies" (PDF). Archived from the original (PDF) on 28 July 2020. Retrieved 16 April 2020.

doi.org (Global: 2^nd place; English: 2^nd place)

Agostini, M.; Altenmüller, K.; et al. (The BOREXINO collaboration) (25 June 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. PMID 33239797. S2CID 227174644.
Schuler, S.C.; King, J.R.; The, L.-S. (2009). "Stellar Nucleosynthesis in the Hyades open cluster". The Astrophysical Journal. 701 (1): 837–849. arXiv:0906.4812. Bibcode:2009ApJ...701..837S. doi:10.1088/0004-637X/701/1/837. S2CID 10626836.
Bethe, Hans A. (1939). "Energy Production in Stars". Physical Review. 55 (1): 541–7. Bibcode:1939PhRv...55..103B. doi:10.1103/PhysRev.55.103. PMID 17835673.
Bethe, Hans A. (1939). "Energy production in stars". Physical Review. 55 (5): 434–456. Bibcode:1939PhRv...55..434B. doi:10.1103/PhysRev.55.434. PMID 17835673.
Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;
Bethe, Hans A.; Bacher, Robert (1936). "Nuclear Physics, A: Stationary states of nuclei" (PDF). Reviews of Modern Physics. 8 (2): 82–229. Bibcode:1936RvMP....8...82B. doi:10.1103/RevModPhys.8.82.
Bethe, Hans A. (1937). "Nuclear Physics, B: Nuclear dynamics, theoretical". Reviews of Modern Physics. 9 (2): 69–244. Bibcode:1937RvMP....9...69B. doi:10.1103/RevModPhys.9.69.
Bethe, Hans A.; Livingston, Milton S. (1937). "Nuclear Physics, C: Nuclear Dynamics, Experimental". Reviews of Modern Physics. 9 (2): 245–390. Bibcode:1937RvMP....9..245L. doi:10.1103/RevModPhys.9.245.
Bardi, Jason Socrates (23 January 2008). "Landmarks: What makes the stars shine?". Physical Review Focus. Vol. 21, no. 3. doi:10.1103/physrevfocus.21.3. Retrieved 26 November 2018.
Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P.; et al. (LUNA Collaboration) (2006). "First measurement of the ¹⁴N(p,γ)¹⁵O cross section down to 70 keV". Physics Letters B. 634 (5–6): 483–487. arXiv:nucl-ex/0602012. Bibcode:2006PhLB..634..483L. doi:10.1016/j.physletb.2006.02.021. S2CID 16875233.
Depalo, R; LUNA collaboration (5 January 2016). "Towards a study of 22 Ne(p γ ) 23 Na at LUNA". Journal of Physics: Conference Series. 665 012017. doi:10.1088/1742-6596/665/1/012017. hdl:2434/931202. ISSN 1742-6588.
Marks and Sarna (December 1998). "The chemical evolution of the secondary stars in close binaries, arising from common-envelope evolution and nova outbursts". Monthly Notices of the Royal Astronomical Society. 301 (3): 699–720. Bibcode:1998MNRAS.301..699M. doi:10.1046/j.1365-8711.1998.02039.x.

handle.net (Global: 102^nd place; English: 76^th place)

hdl.handle.net

Depalo, R; LUNA collaboration (5 January 2016). "Towards a study of 22 Ne(p γ ) 23 Na at LUNA". Journal of Physics: Conference Series. 665 012017. doi:10.1088/1742-6596/665/1/012017. hdl:2434/931202. ISSN 1742-6588.

harvard.edu (Global: 18^th place; English: 17^th place)

ui.adsabs.harvard.edu

Agostini, M.; Altenmüller, K.; et al. (The BOREXINO collaboration) (25 June 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. PMID 33239797. S2CID 227174644.
Schuler, S.C.; King, J.R.; The, L.-S. (2009). "Stellar Nucleosynthesis in the Hyades open cluster". The Astrophysical Journal. 701 (1): 837–849. arXiv:0906.4812. Bibcode:2009ApJ...701..837S. doi:10.1088/0004-637X/701/1/837. S2CID 10626836.
Bethe, Hans A. (1939). "Energy Production in Stars". Physical Review. 55 (1): 541–7. Bibcode:1939PhRv...55..103B. doi:10.1103/PhysRev.55.103. PMID 17835673.
Bethe, Hans A. (1939). "Energy production in stars". Physical Review. 55 (5): 434–456. Bibcode:1939PhRv...55..434B. doi:10.1103/PhysRev.55.434. PMID 17835673.
Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;
Bethe, Hans A.; Bacher, Robert (1936). "Nuclear Physics, A: Stationary states of nuclei" (PDF). Reviews of Modern Physics. 8 (2): 82–229. Bibcode:1936RvMP....8...82B. doi:10.1103/RevModPhys.8.82.
Bethe, Hans A. (1937). "Nuclear Physics, B: Nuclear dynamics, theoretical". Reviews of Modern Physics. 9 (2): 69–244. Bibcode:1937RvMP....9...69B. doi:10.1103/RevModPhys.9.69.
Bethe, Hans A.; Livingston, Milton S. (1937). "Nuclear Physics, C: Nuclear Dynamics, Experimental". Reviews of Modern Physics. 9 (2): 245–390. Bibcode:1937RvMP....9..245L. doi:10.1103/RevModPhys.9.245.
Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P.; et al. (LUNA Collaboration) (2006). "First measurement of the ¹⁴N(p,γ)¹⁵O cross section down to 70 keV". Physics Letters B. 634 (5–6): 483–487. arXiv:nucl-ex/0602012. Bibcode:2006PhLB..634..483L. doi:10.1016/j.physletb.2006.02.021. S2CID 16875233.
Marks and Sarna (December 1998). "The chemical evolution of the secondary stars in close binaries, arising from common-envelope evolution and nova outbursts". Monthly Notices of the Royal Astronomical Society. 301 (3): 699–720. Bibcode:1998MNRAS.301..699M. doi:10.1046/j.1365-8711.1998.02039.x.

in2p3.fr (Global: low place; English: low place)

amdc.in2p3.fr

Wapstra, Aaldert; Audi, Georges (18 November 2003). "The 2003 Atomic Mass Evaluation". Atomic Mass Data Center. Archived from the original on 28 September 2011. Retrieved 25 October 2011.

iop.org (Global: 1,725^th place; English: 1,828^th place)

iopscience.iop.org

Depalo, R; LUNA collaboration (5 January 2016). "Towards a study of 22 Ne(p γ ) 23 Na at LUNA". Journal of Physics: Conference Series. 665 012017. doi:10.1088/1742-6596/665/1/012017. hdl:2434/931202. ISSN 1742-6588.

nature.com (Global: 234^th place; English: 397^th place)

Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;

nih.gov (Global: 4^th place; English: 4^th place)

pubmed.ncbi.nlm.nih.gov

Agostini, M.; Altenmüller, K.; et al. (The BOREXINO collaboration) (25 June 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. PMID 33239797. S2CID 227174644.
Bethe, Hans A. (1939). "Energy Production in Stars". Physical Review. 55 (1): 541–7. Bibcode:1939PhRv...55..103B. doi:10.1103/PhysRev.55.103. PMID 17835673.
Bethe, Hans A. (1939). "Energy production in stars". Physical Review. 55 (5): 434–456. Bibcode:1939PhRv...55..434B. doi:10.1103/PhysRev.55.434. PMID 17835673.
Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;

phys.org (Global: 1,283^rd place; English: 1,130^th place)

"Neutrinos yield first experimental evidence of catalyzed fusion dominant in many stars". phys.org. Retrieved 26 November 2020. Pocar points out, "Confirmation of CNO burning in our sun, where it operates at only one percent, reinforces our confidence that we understand how stars work."

semanticscholar.org (Global: 11^th place; English: 8^th place)

api.semanticscholar.org

Agostini, M.; Altenmüller, K.; et al. (The BOREXINO collaboration) (25 June 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. PMID 33239797. S2CID 227174644.
Schuler, S.C.; King, J.R.; The, L.-S. (2009). "Stellar Nucleosynthesis in the Hyades open cluster". The Astrophysical Journal. 701 (1): 837–849. arXiv:0906.4812. Bibcode:2009ApJ...701..837S. doi:10.1088/0004-637X/701/1/837. S2CID 10626836.
Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;
Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P.; et al. (LUNA Collaboration) (2006). "First measurement of the ¹⁴N(p,γ)¹⁵O cross section down to 70 keV". Physics Letters B. 634 (5–6): 483–487. arXiv:nucl-ex/0602012. Bibcode:2006PhLB..634..483L. doi:10.1016/j.physletb.2006.02.021. S2CID 16875233.

web.archive.org (Global: 1^st place; English: 1^st place)

Wapstra, Aaldert; Audi, Georges (18 November 2003). "The 2003 Atomic Mass Evaluation". Atomic Mass Data Center. Archived from the original on 28 September 2011. Retrieved 25 October 2011.
Depalo, Rosanna. "The neon-sodium cycle: Study of the 22Ne(p, γ)23Na reaction at astrophysical energies" (PDF). Archived from the original (PDF) on 28 July 2020. Retrieved 16 April 2020.

worldcat.org (Global: 5^th place; English: 5^th place)

search.worldcat.org

Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J.; Biondi, R.; Bravo, D.; Caccianiga, B. (25 November 2020). "Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun". Nature. 587 (7835): 577–582. arXiv:2006.15115. Bibcode:2020Natur.587..577B. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. PMID 33239797. S2CID 227174644. This result therefore paves the way towards a direct measurement of the solar metallicity using CNO neutrinos. Our findings quantify the relative contribution of CNO fusion in the Sun to be of the order of 1 per cent;
Depalo, R; LUNA collaboration (5 January 2016). "Towards a study of 22 Ne(p γ ) 23 Na at LUNA". Journal of Physics: Conference Series. 665 012017. doi:10.1088/1742-6596/665/1/012017. hdl:2434/931202. ISSN 1742-6588.

CNO cycle (English Wikipedia)

aps.org (Global: 1,503rd place; English: 1,378th place)

physics.aps.org

archive.org (Global: 6th place; English: 6th place)

arxiv.org (Global: 69th place; English: 59th place)

books.google.com (Global: 3rd place; English: 3rd place)

caltech.edu (Global: 887th place; English: 714th place)

authors.library.caltech.edu

core.ac.uk (Global: 1,734th place; English: 1,312th place)

doi.org (Global: 2nd place; English: 2nd place)

handle.net (Global: 102nd place; English: 76th place)