Κύκλος CNO (Greek Wikipedia)

Analysis of information sources in references of the Wikipedia article "Κύκλος CNO" in Greek language version.

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9doi.org

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7harvard.edu

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4archive.org

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2nih.gov

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2web.archive.org

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1arxiv.org

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1nature.com

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1worldcat.org

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1phys.org

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1caltech.edu

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1aps.org

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1in2p3.fr

low place

1core.ac.uk

1,734^th place

803^rd place

aps.org

physics.aps.org

Bardi, Jason Socrates (January 23, 2008). «Landmarks: What makes the stars shine?». Physical Review Focus 21 (3). doi:10.1103/physrevfocus.21.3. https://physics.aps.org/story/v21/st3. Ανακτήθηκε στις November 26, 2018.

archive.org

Salaris, Maurizio· Cassisi, Santi (2005). Evolution of Stars and Stellar Populations. John Wiley and Sons. σελίδες 119–121. ISBN 0-470-09220-3.
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 έκδοση). Springer Science & Business Media. σελίδες 108–111. ISBN 3-540-25124-3.
Bethe, Hans A. (1939). «Energy production in stars». Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. PMID 17835673. Bibcode: 1939PhRv...55..434B. https://archive.org/details/sim_physical-review_1939-03-01_55_5/page/n9.
Krane, Kenneth S. (1988). Introductory Nuclear Physics. John Wiley & Sons. σελ. 537. ISBN 0-471-80553-X.

arxiv.org

Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J. και άλλοι. (25 June 2020). «First Direct Experimental Evidenceof CNO neutrinos» (στα αγγλικά).
arXiv:2006.15115
[hep-ex]
.

caltech.edu

authors.library.caltech.edu

Bethe, Hans A.; Bacher, Robert (1936). «Nuclear Physics, A: Stationary states of nuclei». Reviews of Modern Physics 8 (2): 82–229. doi:10.1103/RevModPhys.8.82. Bibcode: 1936RvMP....8...82B. https://authors.library.caltech.edu/51288/1/RevModPhys.8.82.pdf.

core.ac.uk

«Αρχειοθετημένο αντίγραφο» (PDF). Αρχειοθετήθηκε από το πρωτότυπο (PDF) στις 28 Ιουλίου 2020. Ανακτήθηκε στις 28 Νοεμβρίου 2020.

doi.org

dx.doi.org

Schuler, S.C.; King, J.R.; The, L.-S. (2009). «Stellar Nucleosynthesis in the Hyades open cluster». The Astrophysical Journal 701 (1): 837–849. doi:10.1088/0004-637X/701/1/837. Bibcode: 2009ApJ...701..837S.
Bethe, Hans A. (1939). «Energy Production in Stars». Physical Review 55 (1): 541–7. doi:10.1103/PhysRev.55.103. PMID 17835673. Bibcode: 1939PhRv...55..103B.
Bethe, Hans A. (1939). «Energy production in stars». Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. PMID 17835673. Bibcode: 1939PhRv...55..434B. https://archive.org/details/sim_physical-review_1939-03-01_55_5/page/n9.
Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J. και άλλοι. (25 November 2020). «Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun» (στα αγγλικά). Nature 587 (7835): 577–582. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. https://www.nature.com/articles/s41586-020-2934-0. «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». Reviews of Modern Physics 8 (2): 82–229. doi:10.1103/RevModPhys.8.82. Bibcode: 1936RvMP....8...82B. https://authors.library.caltech.edu/51288/1/RevModPhys.8.82.pdf.
Bethe, Hans A. (1937). «Nuclear Physics, B: Nuclear dynamics, theoretical». Reviews of Modern Physics 9 (2): 69–244. doi:10.1103/RevModPhys.9.69. Bibcode: 1937RvMP....9...69B.
Bethe, Hans A.; Livingston, Milton S. (1937). «Nuclear Physics, C: Nuclear Dynamics, Experimental». Reviews of Modern Physics 9 (2): 245–390. doi:10.1103/RevModPhys.9.245. Bibcode: 1937RvMP....9..245L.
Bardi, Jason Socrates (January 23, 2008). «Landmarks: What makes the stars shine?». Physical Review Focus 21 (3). doi:10.1103/physrevfocus.21.3. https://physics.aps.org/story/v21/st3. Ανακτήθηκε στις November 26, 2018.
Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P. και άλλοι. (2006). «First measurement of the ¹⁴N(p,γ)¹⁵O cross section down to 70 keV». Physics Letters B 634 (5–6): 483–487. doi:10.1016/j.physletb.2006.02.021. Bibcode: 2006PhLB..634..483L.

harvard.edu

adsabs.harvard.edu

Schuler, S.C.; King, J.R.; The, L.-S. (2009). «Stellar Nucleosynthesis in the Hyades open cluster». The Astrophysical Journal 701 (1): 837–849. doi:10.1088/0004-637X/701/1/837. Bibcode: 2009ApJ...701..837S.
Bethe, Hans A. (1939). «Energy Production in Stars». Physical Review 55 (1): 541–7. doi:10.1103/PhysRev.55.103. PMID 17835673. Bibcode: 1939PhRv...55..103B.
Bethe, Hans A. (1939). «Energy production in stars». Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. PMID 17835673. Bibcode: 1939PhRv...55..434B. https://archive.org/details/sim_physical-review_1939-03-01_55_5/page/n9.
Bethe, Hans A.; Bacher, Robert (1936). «Nuclear Physics, A: Stationary states of nuclei». Reviews of Modern Physics 8 (2): 82–229. doi:10.1103/RevModPhys.8.82. Bibcode: 1936RvMP....8...82B. https://authors.library.caltech.edu/51288/1/RevModPhys.8.82.pdf.
Bethe, Hans A. (1937). «Nuclear Physics, B: Nuclear dynamics, theoretical». Reviews of Modern Physics 9 (2): 69–244. doi:10.1103/RevModPhys.9.69. Bibcode: 1937RvMP....9...69B.
Bethe, Hans A.; Livingston, Milton S. (1937). «Nuclear Physics, C: Nuclear Dynamics, Experimental». Reviews of Modern Physics 9 (2): 245–390. doi:10.1103/RevModPhys.9.245. Bibcode: 1937RvMP....9..245L.
Lemut, A.; Bemmerer, D.; Confortola, F.; Bonetti, R.; Broggini, C.; Corvisiero, P. και άλλοι. (2006). «First measurement of the ¹⁴N(p,γ)¹⁵O cross section down to 70 keV». Physics Letters B 634 (5–6): 483–487. doi:10.1016/j.physletb.2006.02.021. Bibcode: 2006PhLB..634..483L.

in2p3.fr

amdc.in2p3.fr

Wapstra, Aaldert· Audi, Georges (18 Νοεμβρίου 2003). «The 2003 Atomic Mass Evaluation». Atomic Mass Data Center. Αρχειοθετήθηκε από το πρωτότυπο στις 28 Σεπτεμβρίου 2011. Ανακτήθηκε στις 25 Οκτωβρίου 2011.

nature.com

Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J. και άλλοι. (25 November 2020). «Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun» (στα αγγλικά). Nature 587 (7835): 577–582. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. https://www.nature.com/articles/s41586-020-2934-0. «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

ncbi.nlm.nih.gov

Bethe, Hans A. (1939). «Energy Production in Stars». Physical Review 55 (1): 541–7. doi:10.1103/PhysRev.55.103. PMID 17835673. Bibcode: 1939PhRv...55..103B.
Bethe, Hans A. (1939). «Energy production in stars». Physical Review 55 (5): 434–456. doi:10.1103/PhysRev.55.434. PMID 17835673. Bibcode: 1939PhRv...55..434B. https://archive.org/details/sim_physical-review_1939-03-01_55_5/page/n9.

phys.org

«Neutrinos yield first experimental evidence of catalyzed fusion dominant in many stars». phys.org (στα Αγγλικά). Ανακτήθηκε στις 26 Νοεμβρίου 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."

web.archive.org

Wapstra, Aaldert· Audi, Georges (18 Νοεμβρίου 2003). «The 2003 Atomic Mass Evaluation». Atomic Mass Data Center. Αρχειοθετήθηκε από το πρωτότυπο στις 28 Σεπτεμβρίου 2011. Ανακτήθηκε στις 25 Οκτωβρίου 2011.
«Αρχειοθετημένο αντίγραφο» (PDF). Αρχειοθετήθηκε από το πρωτότυπο (PDF) στις 28 Ιουλίου 2020. Ανακτήθηκε στις 28 Νοεμβρίου 2020.

worldcat.org

Agostini, M.; Altenmüller, K.; Appel, S.; Atroshchenko, V.; Bagdasarian, Z.; Basilico, D.; Bellini, G.; Benziger, J. και άλλοι. (25 November 2020). «Experimental evidence of neutrinos produced in the CNO fusion cycle in the Sun» (στα αγγλικά). Nature 587 (7835): 577–582. doi:10.1038/s41586-020-2934-0. ISSN 1476-4687. https://www.nature.com/articles/s41586-020-2934-0. «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;».