HASH: the Hong Kong/AAO/Strasbourg Hα planetary nebula database
- 1. Department of Physics, The University of Hong Kong, Hong Kong SAR (China)
Description
By incorporating our major recent discoveries with re-measured and verified contents of existing catalogues we provide, for the first time, an accessible, reliable, on-line SQL database for essential, up-to date information for all known Galactic planetary nebulae (PNe). We have attempted to: i) reliably remove PN mimics/false ID's that have biased previous studies and ii) provide accurate positions, sizes, morphologies, multi-wavelength imagery and spectroscopy. We also provide a link to CDS/Vizier for the archival history of each object and other valuable links to external data. With the HASH interface, users can sift, select, browse, collate, investigate, download and visualise the entire currently known Galactic PNe diversity. HASH provides the community with the most complete and reliable data with which to undertake new science. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1742-6596/728/3/032008Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Physics. Conference Series (Online)
- Journal Volume
- 728
- Journal Issue
- 3
- Journal Page Range
- [10 p.]
- ISSN
- 1742-6596
Conference
- Title
- Physics and chemistry of the late stages of stellar evolution
- Acronym
- 11. Pacific Rim conference on stellar astrophysics
- Dates
- 14-17 Dec 2015
- Place
- Hong Kong (China)
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 48100354
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; CADMIUM SULFIDES; CATALOGS; INTERFACES; MILKY WAY; MORPHOLOGY; PLANETARY NEBULAE; WAVELENGTHS
- Descriptors DEC
- CADMIUM COMPOUNDS; CHALCOGENIDES; DOCUMENT TYPES; GALAXIES; INORGANIC PHOSPHORS; NEBULAE; PHOSPHORS; PHYSICS; SULFIDES; SULFUR COMPOUNDS