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- ...bout 500,000 years.<ref>{{Cite book|title = The Evolution of Protostars in Protostars and Planets VI |display-authors=etal |author1=Dunham, M. M. |publisher = Un ...ibcode = 1980ApJ...241..637S }}</ref> clarified the issue, and showed that protostars are only modestly larger than main-sequence stars of the same mass. This ba ...10 KB (1,422 words) - 03:26, 24 May 2025
- 2 KB (227 words) - 07:39, 3 February 2025
- * ''[[Protostars (book)|Protostars]]'' (1971) (with [[David Gerrold]]) ...5 KB (584 words) - 00:14, 15 January 2025
- ...stars have no pre-main-sequence stage because they contract too quickly as protostars. By the time they become visible, the hydrogen in their centers is already ...4 KB (540 words) - 02:20, 30 August 2024
- *Structure of magnetic fields in protostars ...5 KB (671 words) - 00:37, 27 May 2025
- ...hant's Trunk Nebula. This pressure has triggered the current generation of protostars.<ref>{{cite journal| last = Barentsen| first = G| title = T Tauri candidate ...5 KB (649 words) - 04:48, 18 June 2025
- ...(2013). [http://adsabs.harvard.edu/abs/2013Ap%26SS.344..175M ''Discovering protostars and their host clusters via WISE''], ApSS, 344, 1</ref> ...6 KB (875 words) - 18:10, 15 March 2025
- [[Protostar|Protostars]] on the Hayashi track are fully convective and due to the large presence o ...5 KB (732 words) - 23:30, 15 March 2025
- ...Feb 07 |publisher=Chandra.harvard.edu |access-date=2012-04-01}}</ref> Any protostars in the pillars' [[List of astronomy acronyms#E|EGGs]] are not yet hot enoug ...11 KB (1,520 words) - 21:47, 9 June 2025
- 8 KB (976 words) - 16:12, 20 May 2025
- ...henomena with shocks being driven by a [[collimation|collimated]] jet from protostars.<ref name="Reipurth1997"/><ref name=Dopita1982/> ...of thousands to about a million years old. The youngest of these are still protostars in the process of collecting from their surrounding gases. Astronomers divi ...36 KB (5,170 words) - 20:11, 15 March 2025
- ...time|free fall timescale]], which is roughly 100,000 years for solar-mass protostars, and ends when the protostar reaches approximately 4000 K. This is known a ...24 KB (3,800 words) - 23:23, 15 March 2025
- | thesis_title = Circumstellar dust: From protostars to planetary systems ...9 KB (1,198 words) - 23:23, 26 May 2025
- ...se cores with spacing comparable to the filament inner width, and embedded protostars with outflows.{{technical inline|date=August 2023}}<ref>{{cite journal |las | title=Protostars and Planets IV | date=2000 ...49 KB (6,865 words) - 09:38, 15 November 2025
- ...D. |last2=Truran |first2=James W. |last3=Williams |first3=Robert E. |title=Protostars and Planets III |date=1993 |publisher=University of Arizona Press |location ...9 KB (1,196 words) - 10:47, 17 April 2025
- 9 KB (1,389 words) - 21:47, 23 May 2025
- ...Before this satellite ran out of [[liquid helium]] in 1998, it discovered protostars and water in our universe (even on Saturn and Uranus).<ref>{{Cite web|url=h ...du/abs/2013Ap%26SS.344..175M|bibcode=2013Ap&SS.344..175M|title=Discovering protostars and their host clusters via WISE|last1=Majaess|first1=D.|journal=Astrophysi ...23 KB (3,105 words) - 15:35, 18 November 2025
- * ''Protostars & Planets: Studies of Star Formation and of the Origin of the Solar System' ...11 KB (1,468 words) - 21:06, 7 June 2025
- ...pilgrimage to the Great Plume of Agosoria. Every eleven years, one of the protostars emits a neutron blast that the pilgrims consider a sacred event. Captain [[ ...12 KB (1,750 words) - 16:50, 23 May 2025
- ...ores with spacing comparable to the filament inner width, and embedded two protostars with gas outflows.<ref>{{cite journal |last1=Zhang |first1=Guo-Yin |last2=A ...(2013). [http://adsabs.harvard.edu/abs/2013Ap%26SS.344..175M ''Discovering protostars and their host clusters via WISE''], ApSS, 344, 1 ([http://vizier.u-strasbg ...50 KB (7,446 words) - 04:11, 15 November 2025