Hα Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks
Fuente:
Redalyc
Guardado en:
| Autor principal: | |
|---|---|
| Formato: | Artículo científico |
| Lenguaje: | en |
| Publicado: |
Universidad Nacional Autónoma de México
2003
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
| _version_ | 1876456987951104000 |
|---|---|
| author | Lorena Arias |
| author_facet | Lorena Arias |
| contents | Hα Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks Lorena Arias Patricia Ambrocio Cruz Eduardo de la Fuente Margarita Rosado Física, Astronomía y Matemáticas Stars: Pre H II Regions Main Sequence Stars: Mass Loss ISM: Individual (Orion Nebula) We summarize the kinematical results obtained from an Hα Fabry-Perot study of some proplyds in the Orion nebula. These results are presented in detail in de la Fuente et al. (2003 a,b). We obtained heliocentric systemic velocities, mass loss rates, disks life-times and radial velocity profiles, finding that Fabry-Perot interferometry constitutes an efective technique for the detection of proplyds. We also present a brief summary of some astrobiological aspects presented by Throop et al. (2001, 2002). We illustrate our results using the proplyds 168-326, 167-317, 163-317, 158-323, 158-327 and 161-314. 2003 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101807 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) Vol.18 |
| format | Artículo científico |
| id | redalyc_57101807 |
| institution | Redalyc |
| language | en |
| publishDate | 2003 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Hα Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks Lorena Arias Física, Astronomía y Matemáticas Stars: Pre H II Regions Main Sequence Stars: Mass Loss ISM: Individual (Orion Nebula) Hα Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks Lorena Arias Patricia Ambrocio Cruz Eduardo de la Fuente Margarita Rosado Física, Astronomía y Matemáticas Stars: Pre H II Regions Main Sequence Stars: Mass Loss ISM: Individual (Orion Nebula) We summarize the kinematical results obtained from an Hα Fabry-Perot study of some proplyds in the Orion nebula. These results are presented in detail in de la Fuente et al. (2003 a,b). We obtained heliocentric systemic velocities, mass loss rates, disks life-times and radial velocity profiles, finding that Fabry-Perot interferometry constitutes an efective technique for the detection of proplyds. We also present a brief summary of some astrobiological aspects presented by Throop et al. (2001, 2002). We illustrate our results using the proplyds 168-326, 167-317, 163-317, 158-323, 158-327 and 161-314. 2003 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57101807 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) Vol.18 |
| title | Hα Fabry-Perot Study in the Orion Nebula (M 42): Protoplanetary Disks |
| topic | Física, Astronomía y Matemáticas Stars: Pre H II Regions Main Sequence Stars: Mass Loss ISM: Individual (Orion Nebula) |
| url | https://www.redalyc.org/articulo.oa?id=57101807 |