Ionization-driven star formation:: the case IR bubble N10 (2016)
- Authors:
- Autor USP: LEPINE, JACQUES RAYMOND DANIEL - IAG
- Unidade: IAG
- Subjects: MEIO INTERESTELAR; FORMAÇÃO DE ESTRELAS
- Language: Inglês
- Imprenta:
- Publisher: UNIVAP
- Publisher place: Campinas, SP
- Date published: 2016
- Source:
- Conference titles: International Symposium and Workshop on Astrochemistry
-
ABNT
GAMA, D et al. Ionization-driven star formation:: the case IR bubble N10. 2016, Anais.. Campinas, SP: UNIVAP, 2016. . Acesso em: 29 jan. 2026. -
APA
Gama, D., Lépine, J. R. D., Lefloch, B., & Mendonza, E. (2016). Ionization-driven star formation:: the case IR bubble N10. In Understanding extraterrestrial molecular complexity through experiments and observations. Campinas, SP: UNIVAP. -
NLM
Gama D, Lépine JRD, Lefloch B, Mendonza E. Ionization-driven star formation:: the case IR bubble N10. Understanding extraterrestrial molecular complexity through experiments and observations. 2016 ;[citado 2026 jan. 29 ] -
Vancouver
Gama D, Lépine JRD, Lefloch B, Mendonza E. Ionization-driven star formation:: the case IR bubble N10. Understanding extraterrestrial molecular complexity through experiments and observations. 2016 ;[citado 2026 jan. 29 ] - Construção de um catálogo de aglomerados abertos para estudo da dinâmica da estrutura espiral da galáxia
- Física dos braços espirais de galáxias
- Numerical models for shocks and wave propagation in dense cloud cores
- A new catalog of open clusters
- New catalogue of optically visible open clusters and candidates
- Constraints on the mass of the dark halo from the rotation curve of the galaxy
- A velocidade da rotação dos braços espirais da Via Láctea
- Fractal 3-d simulations of molecular clouds
- Model of the galaxy for predicting star counts in the infrared
- Models for the 3D axisymmetric gravitational potential of the Milky Way galaxy: a detailed modelling of the Galactic disk
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