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A search for diffuse bands in the circumstellar envelopes of post-AGB stars

Author
LUNA, R1 ; COX, N. L. J2 ; SATORRE, M. A1 ; GARCIA HERNANDEZ, D. A3 ; SUAREZ, O4 ; GARCIA LARIO, P2
[1] Laboratorio de Astrofísica Expérimental, Escuela Politécnica Superior de Alcoy, Universidad Politécnica de Valencia, Plaza de Ferrándiz y Carbonell, 03801 Alcoy, Alicante, Spain
[2] Herschel Science Centre, Research and Scientific Support Department of ESA, European Space Astronomy Centre, PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
[3] W. J. McDonald Observatory. The University of Texas at Austin. 1 University Station, C1400, Austin, TX 78712-0259, United States
[4] LUAN, Université de Nice Sophia Antipolis, Parc Valrose, 06108 Nice, France
Source

Astronomy and astrophysics (Berlin. Print). 2008, Vol 480, Num 1, pp 133-148, 16 p ; ref : 3/4 p

CODEN
AAEJAF
ISSN
0004-6361
Scientific domain
Astronomy earth cosmic environment
Publisher
EDP Sciences, Les Ulis
Publication country
France
Document type
Article
Language
English
Author keyword
ISM: dust, extinction stars: AGB and post-AGB
Keyword (fr)
Branche géante asymptotique Déplacement Doppler Enveloppe circumstellaire Excitation Matière interstellaire Rougissement interstellaire Spectrométrie optique Type spectral Vitesse radiale
Keyword (en)
Asymptotic giant branch Doppler shift Circumstellar shells Excitation Interstellar matter Interstellar reddening Optical spectrometry Spectral type Radial velocity
Keyword (es)
Rama gigante asintótica Espectrometría óptica Tipo espectral
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20121843

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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