Херцшпрунг-Раселов дијаграм: Разлика помеѓу преработките
| [непроверена преработка] | [непроверена преработка] |
Избришана содржина Додадена содржина
Мала промена |
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Ред 57:
== Наводи ==
{{reflist}}
== Референци ==
* {{cite journal
| last = Casagrande | first = L. | coauthors = Portinari, L., and Flynn, C.
| year = 2006 | month = November
| title = Accurate fundamental parameters for lower main-sequence stars
| journal = MNRAS | volume = 373 | issue = 1 | pages = 13–44
| doi =10.1111/j.1365-2966.2006.10999.x
| url = http://adsabs.harvard.edu/abs/2006astro.ph..8504C
| format = Abstract | accessdate = 2007-02-06 }}
* {{cite book
| last = Porter | first = Roy
| title = The Cambridge History of Science
| publisher = Cambridge University Press
| date = 2003 | location = Cambridge, UK
| pages = 518 | isbn = 978-0521572439 }}
* {{cite journal
| last = Sekiguchi | first = Maki | coauthors = Fukugita, Masataka
| year = 2000 | month = August | title = A Study of the B-V Color-Temperature Relation
| journal = The Astronomical Journal | volume = 120 | issue=2 | pages = 1072–1084
| id =
| url =http://www.iop.org/EJ/article/1538-3881/120/2/1072/990160.html
| format=HTML | accessdate = 2008-09-14 | doi = 10.1086/301490 }}
* {{cite book
| last = Smith | first = Robert
| title = Observational Astrophysics
| publisher = Cambridge University Press
| date = 1995 | location = Cambridge, UK
| pages = 236 | isbn = 978-0521278348 }}
== Надворешни врски ==
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