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Exploiting the HASH Planetary Nebula Research Platform

Published online by Cambridge University Press:  08 August 2017

Quentin A. Parker ,
Ivan Bojičić  and
David J. Frew
Quentin A. Parker
Affiliation:
The University of Hong Kong, Department of Physics, Hong Kong SAR, China The University of Hong Kong, Laboratory for Space Research, Hong Kong SAR, China email: quentinp@hku.hk
Ivan Bojičić
Affiliation:
The University of Hong Kong, Department of Physics, Hong Kong SAR, China The University of Hong Kong, Laboratory for Space Research, Hong Kong SAR, China email: quentinp@hku.hk
David J. Frew
Affiliation:
The University of Hong Kong, Department of Physics, Hong Kong SAR, China The University of Hong Kong, Laboratory for Space Research, Hong Kong SAR, China email: quentinp@hku.hk
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Abstract

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The HASH (Hong Kong/ AAO/ Strasbourg/ Hα) planetary nebula research platform is a unique data repository with a graphical interface and SQL capability that offers the community powerful, new ways to undertake Galactic PN studies. HASH currently contains multi-wavelength images, spectra, positions, sizes, morphologies and other data whenever available for 2401 true, 447 likely, and 692 possible Galactic PNe, for a total of 3540 objects. An additional 620 Galactic post-AGB stars, pre-PNe, and PPN candidates are included. All objects were classified and evaluated following the precepts and procedures established and developed by our group over the last 15 years. The complete database contains over 6,700 Galactic objects including the many mimics and related phenomena previously mistaken or confused with PNe. Curation and updating currently occurs on a weekly basis to keep the repository as up to date as possible until the official release of HASH v1 planned in the near future.

Keywords

Planetary nebulaemulti-wavelength imageryspectroscopydatabaseslate-stage stellar evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 36 - 39
Copyright
Copyright © International Astronomical Union 2017 

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