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Planetary Nebulae Detected in the AKARI Far-IR All-Sky Survey Maps

Published online by Cambridge University Press:  30 December 2019

Toshiya Ueta ,
Ryszard Szczerba ,
Andrew G. Fullard  and
Satoshi Takita
Toshiya Ueta
Affiliation:
University of Denver, Denver, CO 80112, U.S.A. email: toshiya.ueta@du.edu (TU)
Ryszard Szczerba
Affiliation:
Nicolaus Copernicus Astronomical Centre, Toruń, Poland,
Andrew G. Fullard
Affiliation:
University of Denver, Denver, CO 80112, U.S.A. email: toshiya.ueta@du.edu (TU)
Satoshi Takita
Affiliation:
National Astronomical Observatory of Japan, Tokyo, Japan
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Abstract

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The AKARI Far-IR All-Sky Survey (AFASS) maps produced by the AKARI Infrared Astronomical Satellite enabled us to probe the far-IR sky for objects having surface brightnesses greater than a few to a couple of dozen MJy sr−1. Recently, we have verified that, if AFASS-measured fluxes are properly corrected for using the aperture correction method based on the empirical point-spread-function templates derived directly from the AFASS maps, point-source photometry measured from the AFASS maps reproduces fluxes in the AKARI bright source catalogue (BSC). We have surveyed the far-IR sky in the AFASS for Galactic planetary nebulae (PNe) based on the University of Hong Kong/Australian Astronomical Observatory/Strasbourg Observatory Hα Planetary Nebula database (HASHPNDB), preliminarily yielding far-IR fluxes for roughly 1000 Galactic PNe including a few hundreds of PNe not listed in the AKARI/BSC.

Keywords

planetary nebulae: generalcircumstellar matterstars: mass lossinfrared: starssurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time , August 2018 , pp. 522 - 524
Copyright
© International Astronomical Union 2019 

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