Please use this identifier to cite or link to this item: https://hdl.handle.net/20.500.12104/42022
Title: H? Fabry-perot study in the Orion nebula (M 42): Protoplanetary disks
Author: De la Fuente, E.
Rosado, M.
Arias, L.
Ambrocio-Cruz, P.
Issue Date: 2003
Abstract: We summarize the kinematical results obtained from an H? 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 profoles, 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.
URI: http://www.scopus.com/inward/record.url?eid=2-s2.0-70649104812&partnerID=40&md5=305d41f4bae078f410e86494aa3fe94d
http://hdl.handle.net/20.500.12104/42022
Appears in Collections:Producción científica UdeG

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