{"@type": "dcat:Dataset", "accessLevel": "public", "accrualPeriodicity": "irregular", "bureauCode": ["026:00"], "contactPoint": {"@type": "vcard:Contact", "fn": "William Henry Lee", "hasEmail": "mailto:wlee@astroscu.unam.mx"}, "describedBy": "http://astrogravs.gsfc.nasa.gov/docs/waveforms/LEE/README", "description": "Gravitational radiation waveforms for black hole-neutron star coalescence calculations. The physical input is Newtonian physics, an ideal gas equation of state with varying compressibility (through the index gamma), and point-mass gravitational radiation back reaction, which is switched off in the simulation once the star is tidally disrupted. All the simulations are 3D, done using SPH.", "distribution": [{"@type": "dcat:Distribution", "downloadURL": "https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns", "format": "HTML", "mediaType": "text/html"}], "identifier": "NASA-0000023", "issued": "2018-06-25", "keyword": ["astronomy", "binary", "black-hole", "gravitational-waves", "ligo", "neutron-stars", "space-science"], "landingPage": "https://asd.gsfc.nasa.gov/archive/astrogravs/docs/catalog.html#bhns", "modified": "2025-03-31", "programCode": ["026:016"], "publisher": {"@type": "org:Organization", "name": "National Aeronautics and Space Administration"}, "temporal": "2000-01-01/2014-01-01", "title": "Black Hole - Neutron Star Binary Mergers"}