R. Bachiller

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Featured researches published by R. Bachiller.

Astronomy and Astrophysics | 2002

P. Cox; P. J. Huggins; J. P. Maillard; E. Habart; C Morisset; R. Bachiller; T. Forveille

We present near-infrared spectro-imaging of the young planetary nebula NGCxa07027 betweenxa02.10 andxa02.20xa0 μ m with high spatial (0.5″) and high spectral (

Astronomy and Astrophysics | 2002

A. Fuente; J. Martin-Pintado; R. Bachiller; A. Rodriguez-Franco; Francesco Palla

rm 8.7 , km , s^{-1}

Astronomy and Astrophysics | 2003

F. Gueth; R. Bachiller; M. Tafalla

) resolution. The observations, made using BEAR at the CFHT, reveal the detailed morphology and kinematics of the ionized nebula (in the Br γ line and 16 other atomic lines) and the surrounding molecular envelope (in the 1–0xa0S(1) line of H 2 ). The observations show that the ionized gas forms an elongated (

Astronomy and Astrophysics | 2004

P. J. Huggins; C. Muthu; R. Bachiller; T. Forveille; P. Cox

{sim} 6 arcsectimes 12arcsec

Astronomy and Astrophysics | 1993

R. Bachiller; P. J. Huggins; P. Cox; T. Forveille

,

Astronomy and Astrophysics | 1992

J. Martin-Pintado; R. Bachiller; A. Fuente

{rm PA} = 32degr

Astronomy and Astrophysics | 1997

R. Bachiller; T. Forveille; P. J. Huggins; P. Cox

), limb-brightened shell with an expansion velocity ofxa019.5xa0u2000along the line of sight. The shell is composed of numerous small condensations and has nearly parallel sides with flattened ends that are not well matched by a uniform ellipsoidal model. Low level Br γ emission is detected at high red- and blue-shifted velocities (

Astronomy and Astrophysics | 1993