Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-23T19:40:14.106Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected] (TU)
Ryszard Szczerba
Affiliation:
Nicolaus Copernicus Astronomical Centre, Toruń, Poland,
Andrew G. Fullard
Affiliation:
University of Denver, Denver, CO 80112, U.S.A. email: [email protected] (TU)
Satoshi Takita
Affiliation:
National Astronomical Observatory of Japan, Tokyo, Japan
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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 

References

Doi, Y., et al. 2015, PASJ, 1503, 6421 Google Scholar
Kawada, M., et al. 2007, PASJ, 59, S389 10.1093/pasj/59.sp2.S389CrossRefGoogle Scholar
Matsuura, S., et al. 2011, ApJ, 737, 2 10.1088/0004-637X/737/1/2CrossRefGoogle Scholar
Murakami, H., et al. 2007, PASJ, 59, S369 10.1093/pasj/59.sp2.S369CrossRefGoogle Scholar
Neugebauer, G., et al. 1984, ApJ, 278, L1 10.1086/184209CrossRefGoogle Scholar
Onaka, T., et al. 2007, PASJ, 59, 401 10.1093/pasj/59.sp2.S401CrossRefGoogle Scholar
Otsuka, M., et al. 2017, ApJS, 231, 22Parker, Q. A., et al. 2017, in IAU Symp. 323, Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution, eds. Liu, X.-W., Stanghellini, L., & Karakas, A., p.36 Google Scholar
Ueta, T., et al. 2018, PASJ, in press (arXiv:1808.00730)Google Scholar
Takita, S., et al. 2015, PASJ, 67, 51 10.1093/pasj/psv033CrossRefGoogle Scholar
Yamamura, I., et al. 2009, in ASP Conf. Ser. Vol. 418, AKARI, a Light to Illuminate the Misty Universe, eds. Onaka, T., White, G. J., Nakagawa, T., & Yamamura, I., p.3 Google Scholar