Impact of initial models and variable accretion rates on the pre-main-sequence evolution of massive and intermediate-mass stars and the early evolution of H ii regions-Reference-Cited by-同舟云学术

Impact of initial models and variable accretion rates on the pre-main-sequence evolution of massive and intermediate-mass stars and the early evolution of H ii regions

Published:2016-03-07 Issue:3 Volume:458 Page:3299-3313
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Mon. Not. R. Astron. Soc.

Author:

Haemmerlé Lionel,Peters Thomas

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/458/3/3299/8007251/stw517.pdf

Reference39 articles.

1. Supersonic turbulence, filamentary accretion and the rapid assembly of massive stars and discs

2. Formation of massive stars by growing accretion rate

3. FLICKERING OF 1.3 cm SOURCES IN SGR B2: TOWARD A SOLUTION TO THE ULTRACOMPACT H II REGION LIFETIME PROBLEM

4. EVIDENCE OF SHORT TIMESCALE FLUX DENSITY VARIATIONS OF UC H II REGIONS IN SGR B2 MAIN AND NORTH

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