Evolution and lifetime of transient clumps in the turbulent interstellar medium (2011)
- Authors:
- Autor USP: GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidade: EACH
- DOI: 10.1088/0004-637X/735/2/99
- Assunto: ASTROFÍSICA ESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: The Astrophysical Journal
- ISSN: 0004-637X
- Volume/Número/Paginação/Ano: v. 735, n. 2, p. 1-7, jul. 2011
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
- Licença: other-oa
-
ABNT
FALCETA GONÇALVES, Diego Antonio e LAZARIAN, A. Evolution and lifetime of transient clumps in the turbulent interstellar medium. The Astrophysical Journal, v. 735, n. 2, p. 1-7, 2011Tradução . . Disponível em: https://doi.org/10.1088/0004-637X/735/2/99. Acesso em: 19 abr. 2024. -
APA
Falceta Gonçalves, D. A., & Lazarian, A. (2011). Evolution and lifetime of transient clumps in the turbulent interstellar medium. The Astrophysical Journal, 735( 2), 1-7. doi:10.1088/0004-637X/735/2/99 -
NLM
Falceta Gonçalves DA, Lazarian A. Evolution and lifetime of transient clumps in the turbulent interstellar medium [Internet]. The Astrophysical Journal. 2011 ; 735( 2): 1-7.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99 -
Vancouver
Falceta Gonçalves DA, Lazarian A. Evolution and lifetime of transient clumps in the turbulent interstellar medium [Internet]. The Astrophysical Journal. 2011 ; 735( 2): 1-7.[citado 2024 abr. 19 ] Available from: https://doi.org/10.1088/0004-637X/735/2/99 - Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics
- On the alignment of PNe and local magnetic field at the Galactic centre: magnetohydrodynamical numerical simulations
- Turbulence in the interstellar medium
- Gas removal in the Ursa Minor Galaxy: linking hydrodynamics and chemical evolution models
- Turbulence in collisionless plasmas: statistical analysis from numerical simulations with pressure anisotropy
- On the origin of interstellar turbulence: less SNe and more galactic dynamics
- Fast magnetic field amplification in the early Universe: growth of collisionless plasma instabilities in turbulent media
- Planck intermediate results: XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
- Radiation hydrodynamic simulations of massive star formation via gravitationally trapped H II regions: spherically symmetric ionized accretion flows
- ASTRI Mini-Array core science at the observatorio del teide
Informações sobre o DOI: 10.1088/0004-637X/735/2/99 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
