فريتز زفيكي (Arabic Wikipedia)

Analysis of information sources in references of the Wikipedia article "فريتز زفيكي" in Arabic language version.

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11wikidata.org

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1wikidata-externalid-url.toolforge.org

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arxiv.org

de Swart، J. G.؛ Bertone، G.؛ van Dongen، J. (2017). "How dark matter came to matter". Nature Astronomy. ج. 1 ع. 59: 0059. arXiv:1703.00013. Bibcode:2017NatAs...1E..59D. DOI:10.1038/s41550-017-0059. S2CID:119092226.

bbc.co.uk

news.bbc.co.uk

"Advancing through a decade". BBC News Online (بالإنجليزية). 31 Dec 2009.

britannica.com

Encyclopædia Britannica | Fritz Zwicky (بالإنجليزية), QID:Q5375741

brockhaus.de

Brockhaus Enzyklopädie | Fritz Zwicky (بالألمانية), QID:Q237227

doi.org

Jürgen Ehlers (18 Nov 2008). "Editorial note to: F. Zwicky The redshift of extragalactic nebulae". General Relativity and Gravitation (بالإنجليزية). 41 (1): 203–206. DOI:10.1007/S10714-008-0706-5. ISSN:0001-7701. Zbl:1162.85305. QID:Q100968438.
F. Zwicky (1954-08). "Energy content of propellants and of explosives". Cellular and Molecular Life Sciences (بالإنجليزية). 10 (8): 326–328. DOI:10.1007/BF02160838. ISSN:1420-9071. QID:Q100968439. {{استشهاد بدورية محكمة}}: تحقق من التاريخ في: |publication-date= (help)
F ZWICKY (1 Dec 1950). "[Intergalactic matter]". Experientia (بالإنجليزية). 6 (12): 441–445. DOI:10.1007/BF02154098. ISSN:0014-4754. PMID:14802391. QID:Q75640475.
Arp, Halton (يونيو 1974). "Fritz Zwicky". Physics Today. ج. 27 ع. 6: 70–71. Bibcode:1974PhT....27f..70A. DOI:10.1063/1.3128662. مؤرشف من الأصل في 2013-09-27.
Zwicky، F. (1933)، "Die Rotverschiebung von extragalaktischen Nebeln"، Helvetica Physica Acta، ج. 6، ص. 110–127، Bibcode:1933AcHPh...6..110Z See also Zwicky، F. (1937)، "On the Masses of Nebulae and of Clusters of Nebulae"، Astrophysical Journal، ج. 86، ص. 217، Bibcode:1937ApJ....86..217Z، DOI:10.1086/143864
Zwicky, F. (1933), "Die Rotverschiebung von extragalaktischen Nebeln" [The red shift of extragalactic neubulae], Helvetica Physica Acta (بالألمانية), vol. 6, pp. 110–127, Bibcode:1933AcHPh...6..110Z, Archived from the original on 2023-12-19 From p 125: "Um, wie beobachtet, einen mittleren Dopplereffekt von 1000 km/sek oder mehr zu erhalten, müsste also die mittlere Dichte im Comasystem mindestens 400 mal grösser sein als die auf Grund von Beobachtungen an leuchtender Materie abgeleitete. Falls sich dies bewahrheiten sollte, würde sich also das überraschende Resultat ergeben, dass dunkle Materie in sehr viel grösserer Dichte vorhanden ist als leuchtende Materie." (In order to obtain an average Doppler effect of 1000 km/s or more, as observed, the average density in the Coma system would thus have to be at least 400 times greater than that derived on the basis of observations of luminous matter. If this were to be verified, the surprising result would then follow that dark matter is present in very much greater density than luminous matter.)
- See also Zwicky، F. (1937)، "On the masses of nebulae and of clusters of nebulae"، Astrophysical Journal، ج. 86، ص. 217، Bibcode:1937ApJ....86..217Z، DOI:10.1086/143864
- de Swart، J. G.؛ Bertone، G.؛ van Dongen، J. (2017). "How dark matter came to matter". Nature Astronomy. ج. 1 ع. 59: 0059. arXiv:1703.00013. Bibcode:2017NatAs...1E..59D. DOI:10.1038/s41550-017-0059. S2CID:119092226.

enciclopedia.cat

Gran Enciclopèdia Catalana | Fritz Zwicky (بالكتالونية), Grup Enciclopèdia, QID:Q2664168

enciklopedija.hr

Dalibor Brozović; Tomislav Ladan (1999), Hrvatska enciklopedija | Fritz Zwicky (بالكرواتية), Leksikografski zavod Miroslav Krleža, OL:120005M, QID:Q1789619

ethz.ch

zwickymeeting.astro.phys.ethz.ch

https://zwickymeeting.astro.phys.ethz.ch/zwicky.php. {{استشهاد ويب}}: |url= بحاجة لعنوان (مساعدة) والوسيط |title= غير موجود أو فارغ (من ويكي بيانات) (مساعدة)

handle.net

hdl.handle.net

Magda Streicher (2013-10), Two fishes in the starry sea : deep-sky delights (بالإنجليزية), Astronomical Society of Southern Africa, vol. 72, pp. 175–180, hdl:10520/EJC145597, QID:Q100655278 {{استشهاد}}: تحقق من التاريخ في: |publication-date= (help)

harvard.edu

ui.adsabs.harvard.edu

Arp, Halton (يونيو 1974). "Fritz Zwicky". Physics Today. ج. 27 ع. 6: 70–71. Bibcode:1974PhT....27f..70A. DOI:10.1063/1.3128662. مؤرشف من الأصل في 2013-09-27.
Zwicky، F. (1933)، "Die Rotverschiebung von extragalaktischen Nebeln"، Helvetica Physica Acta، ج. 6، ص. 110–127، Bibcode:1933AcHPh...6..110Z See also Zwicky، F. (1937)، "On the Masses of Nebulae and of Clusters of Nebulae"، Astrophysical Journal، ج. 86، ص. 217، Bibcode:1937ApJ....86..217Z، DOI:10.1086/143864
Zwicky, F. (1933), "Die Rotverschiebung von extragalaktischen Nebeln" [The red shift of extragalactic neubulae], Helvetica Physica Acta (بالألمانية), vol. 6, pp. 110–127, Bibcode:1933AcHPh...6..110Z, Archived from the original on 2023-12-19 From p 125: "Um, wie beobachtet, einen mittleren Dopplereffekt von 1000 km/sek oder mehr zu erhalten, müsste also die mittlere Dichte im Comasystem mindestens 400 mal grösser sein als die auf Grund von Beobachtungen an leuchtender Materie abgeleitete. Falls sich dies bewahrheiten sollte, würde sich also das überraschende Resultat ergeben, dass dunkle Materie in sehr viel grösserer Dichte vorhanden ist als leuchtende Materie." (In order to obtain an average Doppler effect of 1000 km/s or more, as observed, the average density in the Coma system would thus have to be at least 400 times greater than that derived on the basis of observations of luminous matter. If this were to be verified, the surprising result would then follow that dark matter is present in very much greater density than luminous matter.)
- See also Zwicky، F. (1937)، "On the masses of nebulae and of clusters of nebulae"، Astrophysical Journal، ج. 86، ص. 217، Bibcode:1937ApJ....86..217Z، DOI:10.1086/143864
- de Swart، J. G.؛ Bertone، G.؛ van Dongen، J. (2017). "How dark matter came to matter". Nature Astronomy. ج. 1 ع. 59: 0059. arXiv:1703.00013. Bibcode:2017NatAs...1E..59D. DOI:10.1038/s41550-017-0059. S2CID:119092226.
articles.adsabs.harvard.edu
- Zwicky, F. (1933), "Die Rotverschiebung von extragalaktischen Nebeln" [The red shift of extragalactic neubulae], Helvetica Physica Acta (بالألمانية), vol. 6, pp. 110–127, Bibcode:1933AcHPh...6..110Z, Archived from the original on 2023-12-19 From p 125: "Um, wie beobachtet, einen mittleren Dopplereffekt von 1000 km/sek oder mehr zu erhalten, müsste also die mittlere Dichte im Comasystem mindestens 400 mal grösser sein als die auf Grund von Beobachtungen an leuchtender Materie abgeleitete. Falls sich dies bewahrheiten sollte, würde sich also das überraschende Resultat ergeben, dass dunkle Materie in sehr viel grösserer Dichte vorhanden ist als leuchtende Materie." (In order to obtain an average Doppler effect of 1000 km/s or more, as observed, the average density in the Coma system would thus have to be at least 400 times greater than that derived on the basis of observations of luminous matter. If this were to be verified, the surprising result would then follow that dark matter is present in very much greater density than luminous matter.)
  - See also Zwicky، F. (1937)، "On the masses of nebulae and of clusters of nebulae"، Astrophysical Journal، ج. 86، ص. 217، Bibcode:1937ApJ....86..217Z، DOI:10.1086/143864

nih.gov

pubmed.ncbi.nlm.nih.gov

F ZWICKY (1 Dec 1950). "[Intergalactic matter]". Experientia (بالإنجليزية). 6 (12): 441–445. DOI:10.1007/BF02154098. ISSN:0014-4754. PMID:14802391. QID:Q75640475.

nmspacemuseum.org

https://www.nmspacemuseum.org/inductee/fritz-zwicky/. اطلع عليه بتاريخ 2023-07-17. {{استشهاد ويب}}: |url= بحاجة لعنوان (مساعدة) والوسيط |title= غير موجود أو فارغ (من ويكي بيانات) (مساعدة)

openlibrary.org

Dalibor Brozović; Tomislav Ladan (1999), Hrvatska enciklopedija | Fritz Zwicky (بالكرواتية), Leksikografski zavod Miroslav Krleža, OL:120005M, QID:Q1789619

physicstoday.org

Arp, Halton (يونيو 1974). "Fritz Zwicky". Physics Today. ج. 27 ع. 6: 70–71. Bibcode:1974PhT....27f..70A. DOI:10.1063/1.3128662. مؤرشف من الأصل في 2013-09-27.

semanticscholar.org

api.semanticscholar.org

de Swart، J. G.؛ Bertone، G.؛ van Dongen، J. (2017). "How dark matter came to matter". Nature Astronomy. ج. 1 ع. 59: 0059. arXiv:1703.00013. Bibcode:2017NatAs...1E..59D. DOI:10.1038/s41550-017-0059. S2CID:119092226.

st-andrews.ac.uk

mathshistory.st-andrews.ac.uk

تاريخ ماكتوتور لأرشيف الرياضيات، QID:Q547473

theage.com.au

"Mine to shed light on dark matter mystery". The Age (بالإنجليزية). 21 Dec 2009.

web.archive.org

Arp, Halton (يونيو 1974). "Fritz Zwicky". Physics Today. ج. 27 ع. 6: 70–71. Bibcode:1974PhT....27f..70A. DOI:10.1063/1.3128662. مؤرشف من الأصل في 2013-09-27.
Zwicky, F. (1933), "Die Rotverschiebung von extragalaktischen Nebeln" [The red shift of extragalactic neubulae], Helvetica Physica Acta (بالألمانية), vol. 6, pp. 110–127, Bibcode:1933AcHPh...6..110Z, Archived from the original on 2023-12-19 From p 125: "Um, wie beobachtet, einen mittleren Dopplereffekt von 1000 km/sek oder mehr zu erhalten, müsste also die mittlere Dichte im Comasystem mindestens 400 mal grösser sein als die auf Grund von Beobachtungen an leuchtender Materie abgeleitete. Falls sich dies bewahrheiten sollte, würde sich also das überraschende Resultat ergeben, dass dunkle Materie in sehr viel grösserer Dichte vorhanden ist als leuchtende Materie." (In order to obtain an average Doppler effect of 1000 km/s or more, as observed, the average density in the Coma system would thus have to be at least 400 times greater than that derived on the basis of observations of luminous matter. If this were to be verified, the surprising result would then follow that dark matter is present in very much greater density than luminous matter.)
- See also Zwicky، F. (1937)، "On the masses of nebulae and of clusters of nebulae"، Astrophysical Journal، ج. 86، ص. 217، Bibcode:1937ApJ....86..217Z، DOI:10.1086/143864

wikidata-externalid-url.toolforge.org

Store norske leksikon | Fritz Zwicky (بالنرويجية البوكمول والنرويجية النينوشك), ISSN:2464-1480, QID:Q746368

wikidata.org

Encyclopædia Britannica | Fritz Zwicky (بالإنجليزية), QID:Q5375741
Brockhaus Enzyklopädie | Fritz Zwicky (بالألمانية), QID:Q237227
Store norske leksikon | Fritz Zwicky (بالنرويجية البوكمول والنرويجية النينوشك), ISSN:2464-1480, QID:Q746368
Gran Enciclopèdia Catalana | Fritz Zwicky (بالكتالونية), Grup Enciclopèdia, QID:Q2664168
Dalibor Brozović; Tomislav Ladan (1999), Hrvatska enciklopedija | Fritz Zwicky (بالكرواتية), Leksikografski zavod Miroslav Krleža, OL:120005M, QID:Q1789619
Magda Streicher (2013-10), Two fishes in the starry sea : deep-sky delights (بالإنجليزية), Astronomical Society of Southern Africa, vol. 72, pp. 175–180, hdl:10520/EJC145597, QID:Q100655278 {{استشهاد}}: تحقق من التاريخ في: |publication-date= (help)
Jürgen Ehlers (18 Nov 2008). "Editorial note to: F. Zwicky The redshift of extragalactic nebulae". General Relativity and Gravitation (بالإنجليزية). 41 (1): 203–206. DOI:10.1007/S10714-008-0706-5. ISSN:0001-7701. Zbl:1162.85305. QID:Q100968438.
F. Zwicky (1954-08). "Energy content of propellants and of explosives". Cellular and Molecular Life Sciences (بالإنجليزية). 10 (8): 326–328. DOI:10.1007/BF02160838. ISSN:1420-9071. QID:Q100968439. {{استشهاد بدورية محكمة}}: تحقق من التاريخ في: |publication-date= (help)
F ZWICKY (1 Dec 1950). "[Intergalactic matter]". Experientia (بالإنجليزية). 6 (12): 441–445. DOI:10.1007/BF02154098. ISSN:0014-4754. PMID:14802391. QID:Q75640475.
تاريخ ماكتوتور لأرشيف الرياضيات، QID:Q547473
Space Pioneers Enshrined (بالإنجليزية), Las Vegas, 6 Oct 1976, p. 6, QID:Q55284879{{استشهاد}}: صيانة الاستشهاد: مكان بدون ناشر (link)

worldcat.org

Store norske leksikon | Fritz Zwicky (بالنرويجية البوكمول والنرويجية النينوشك), ISSN:2464-1480, QID:Q746368
Jürgen Ehlers (18 Nov 2008). "Editorial note to: F. Zwicky The redshift of extragalactic nebulae". General Relativity and Gravitation (بالإنجليزية). 41 (1): 203–206. DOI:10.1007/S10714-008-0706-5. ISSN:0001-7701. Zbl:1162.85305. QID:Q100968438.
F. Zwicky (1954-08). "Energy content of propellants and of explosives". Cellular and Molecular Life Sciences (بالإنجليزية). 10 (8): 326–328. DOI:10.1007/BF02160838. ISSN:1420-9071. QID:Q100968439. {{استشهاد بدورية محكمة}}: تحقق من التاريخ في: |publication-date= (help)
F ZWICKY (1 Dec 1950). "[Intergalactic matter]". Experientia (بالإنجليزية). 6 (12): 441–445. DOI:10.1007/BF02154098. ISSN:0014-4754. PMID:14802391. QID:Q75640475.

zbmath.org

Jürgen Ehlers (18 Nov 2008). "Editorial note to: F. Zwicky The redshift of extragalactic nebulae". General Relativity and Gravitation (بالإنجليزية). 41 (1): 203–206. DOI:10.1007/S10714-008-0706-5. ISSN:0001-7701. Zbl:1162.85305. QID:Q100968438.

فريتز زفيكي (Arabic Wikipedia)

arxiv.org

bbc.co.uk

news.bbc.co.uk

britannica.com

brockhaus.de

doi.org

enciclopedia.cat

enciklopedija.hr

ethz.ch

zwickymeeting.astro.phys.ethz.ch

handle.net

hdl.handle.net

harvard.edu

ui.adsabs.harvard.edu

articles.adsabs.harvard.edu

nih.gov

pubmed.ncbi.nlm.nih.gov

nmspacemuseum.org

openlibrary.org

physicstoday.org

semanticscholar.org

api.semanticscholar.org

st-andrews.ac.uk

mathshistory.st-andrews.ac.uk

theage.com.au

web.archive.org

wikidata-externalid-url.toolforge.org

wikidata.org

worldcat.org

zbmath.org