An AKARI-FIS Survey of Post-AGB Stars and (Proto) Planetary Nebulae: an Analysis of Extended Emission and the Spectral Energy Distribution

Bibcode
2009ASPC..418..137C
Cox, N.; García-Lario, P.; García-Hernández, D. A.; Manchado, A.
Referencia bibliográfica

AKARI, a Light to Illuminate the Misty Universe ASP Conference Series, Vol. 418, proceedings of a conference held 16-19 February 2009 at the University of Tokyo, Tokyo, Japan. Edited by Takashi Onaka, Glenn J. White, Takao Nakagawa, and Issei Yamamura. San Francisco: Astronomical Society of the Pacific, 2009, p.137

Fecha de publicación:
12
2009
Número de autores
4
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
We present first preliminary results from AKARI/FIS pointed observations of post-AGB stars and planetary nebulae (PNe). A first analysis of the radial (azimuthally averaged) profile of the observed sources shows no evidence for excess emission due to the presence of circumstellar dust. No (detached) circumstellar faint dust-shells are seen in the image maps. Also, we present here first results of aperture flux photometry at wavelengths of 65, 90, 140 and 160 μm. Results are compared with IRAS flux densities as well as the β release of the FIS Bright Source Catalog. Finally, spectral energy distributions are given, by way of an example, for two individual targets in our sample.
Tipo
Sin árbitro

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