Turbulence in the interstellar medium (2014)
- Authors:
- Autor USP: GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidade: EACH
- DOI: 10.5194/npg-21-587-2014
- Subjects: TURBULÊNCIA; MEIO INTERESTELAR; CAMPO MAGNÉTICO
- Language: Inglês
- Imprenta:
- Publisher place: Goettingen
- Date published: 2014
- Source:
- Título do periódico: Nonlinear Processes in Geophysics
- ISSN: 1023-5809
- Volume/Número/Paginação/Ano: v. 21, n. 3, p. 587-604, 2014
- Este periódico é de acesso aberto
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: gold
- Licença: cc-by
-
ABNT
FALCETA GONÇALVES, Diego Antonio et al. Turbulence in the interstellar medium. Nonlinear Processes in Geophysics, v. 21, n. 3, p. 587-604, 2014Tradução . . Disponível em: https://doi.org/10.5194/npg-21-587-2014. Acesso em: 04 ago. 2024. -
APA
Falceta Gonçalves, D. A., Kowal, G., Falgarone, E., & Chian, A. C. L. (2014). Turbulence in the interstellar medium. Nonlinear Processes in Geophysics, 21( 3), 587-604. doi:10.5194/npg-21-587-2014 -
NLM
Falceta Gonçalves DA, Kowal G, Falgarone E, Chian ACL. Turbulence in the interstellar medium [Internet]. Nonlinear Processes in Geophysics. 2014 ; 21( 3): 587-604.[citado 2024 ago. 04 ] Available from: https://doi.org/10.5194/npg-21-587-2014 -
Vancouver
Falceta Gonçalves DA, Kowal G, Falgarone E, Chian ACL. Turbulence in the interstellar medium [Internet]. Nonlinear Processes in Geophysics. 2014 ; 21( 3): 587-604.[citado 2024 ago. 04 ] Available from: https://doi.org/10.5194/npg-21-587-2014 - 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
- 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
- Statistics of reconnection-driven turbulence
- Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor
- Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium
- Planck intermediate results: XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
Informações sobre o DOI: 10.5194/npg-21-587-2014 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas