Plimni rep: razlika između inačica
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Nema sažetka uređivanja |
Kako ovo nitko nije primjetio? |
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Redak 6:
== Povijest ==
Pojavu koju danas nazivamo plimni rep prvi je naširoko proučavao [[Fritz Zwicky]] 1953. godine<ref>(eng.) {{cite journal | title = Luminous and dark formations of intergalactic matter | author = Zwicky, Fritz | journal = [[Physics Today]] | date = travanj 1953. | volume = 6 | issue = 4 | pages = 7–11 | doi = 10.1063/1.3061224|bibcode = 1953PhT.....6....7Z }}</ref> Nekoliko je astrofizičara izrazilo svoje dvojbe da se ova proširenja mogu pojaviti samostalno kao rezultat plimnih sila,<ref>(eng.) {{cite journal | title = The Possibility of a Long Lifetime for Intergalactic Arms | author = Zasov, A. V. | journal = Soviet Astronomy – AJ | volume = 11 | issue = 5 | date = 1968 | bibcode = 1968SvA....11..785Z}}</ref><ref>(eng.) {{cite book | title = Cosmic rays and radio waves as manifestations of a hot universe | author = Gold, T. | author2 = Hoyle, F. | last-author-amp = yes | booktitle = Paris Symposium on Radio Astronomy | publisher = Stanford University Press | pages = 583–588 | url = http://books.google.com/books?id=g56aAAAAIAAJ&pg=PA583&lpg=PA583&dq=paris+symposium+on+radio+astronomy+gold+hoyle&source=bl&ots=1tbiV1-YOy&sig=LwVdsRXnLZq_PfT3Bq9TUBvyICQ&hl=en&ei=Z3kbTIKpJoKBlAeP-eXfCQ&sa=X&oi=book_result&ct=result&resnum=1&ved=0CBIQ6AEwAA#v=onepage&q&f=false | date = 1959.}}</ref>
== Izvori ==
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