Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind
Fuente:
Redalyc
Guardado en:
| Autor principal: | |
|---|---|
| Formato: | Artículo científico |
| Lenguaje: | en |
| Publicado: |
Universidad Nacional Autónoma de México
2004
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1876460796122234880 |
|---|---|
| author | S. Mendoza |
| author_facet | S. Mendoza |
| contents | Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind S. Mendoza J. Cantó A. C. Raga Física, Astronomía y Matemáticas ACCRETION SHOCK WAVES HYDRODYNAMICS Molecular clouds in the interstellar medium suffer gravitational instabilitiesthat lead to the formation of one or multiple stars. A recently formed star insidea cold cloud communicates its gravitational force to the surrounding environmentand soon an accretion flow falling into the star develops. After their formation, allstars soon eject a wind of gas that interacts with the external accretion flow. Thisinteraction produces a shock wave that evolves with time. The work presented inthis article formulates a simple prescription for the evolution of this interaction.With the aid of this model we construct a few radio continuum maps of the source. 2004 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57140203 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.40 |
| format | Artículo científico |
| id | redalyc_57140203 |
| institution | Redalyc |
| language | en |
| publishDate | 2004 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind S. Mendoza Física, Astronomía y Matemáticas ACCRETION SHOCK WAVES HYDRODYNAMICS Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind S. Mendoza J. Cantó A. C. Raga Física, Astronomía y Matemáticas ACCRETION SHOCK WAVES HYDRODYNAMICS Molecular clouds in the interstellar medium suffer gravitational instabilitiesthat lead to the formation of one or multiple stars. A recently formed star insidea cold cloud communicates its gravitational force to the surrounding environmentand soon an accretion flow falling into the star develops. After their formation, allstars soon eject a wind of gas that interacts with the external accretion flow. Thisinteraction produces a shock wave that evolves with time. The work presented inthis article formulates a simple prescription for the evolution of this interaction.With the aid of this model we construct a few radio continuum maps of the source. 2004 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57140203 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.40 |
| title | Hydrodynamical Interaction between an Accretion Flow and a Stellar Wind |
| topic | Física, Astronomía y Matemáticas ACCRETION SHOCK WAVES HYDRODYNAMICS |
| url | https://www.redalyc.org/articulo.oa?id=57140203 |