Hi global scaling relations in the wise-whisp survey

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dc.contributor.authorNaluminsa, Elizabeth
dc.contributor.authorElson, Edward
dc.contributor.authorJarrett, Thomas
dc.date.accessioned2022-07-19T12:38:28Z
dc.date.available2022-07-19T12:38:28Z
dc.date.issued2021
dc.description.abstractWe present the global scaling relations between the neutral atomic hydrogen gas, the stellar disk and the star forming disk in a sample of 228 nearby galaxies that are both spatially and spectrally resolved in HI line emission. We have used HI data from the Westerbork survey of HI in Irregular and Spiral galaxies (WHISP) and Mid Infrared (3.4 µm, 11.6 µm) data from the Wide-field Infrared Survey Explorer (WISE) survey, combining two datasets that are well-suited to such a study in terms of uniformity, resolution and sensitivity. We utilize a novel method of deriving scaling relations for quantities enclosed within the stellar disk rather than integrating over the HI disk and find the global scaling relations to be tighter when defined for enclosed quantities. We also present new HI intensity maps for the WHISP survey derived using a robust noise rejection technique along with corresponding velocity fields.en_US
dc.identifier.citationNaluminsa, E. et al. (2021). Hi global scaling relations in the wise-whisp survey. Monthly Notices of the Royal Astronomical Society, 502(4), 5711 - 5725. 10.1093/mnras/stab067en_US
dc.identifier.issn1365-2966
dc.identifier.uri10.1093/mnras/stab067
dc.identifier.urihttp://hdl.handle.net/10566/7614
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.subjectGalaxiesen_US
dc.subjectAstronomyen_US
dc.subjectPhysicsen_US
dc.subjectDwarfen_US
dc.titleHi global scaling relations in the wise-whisp surveyen_US
dc.typeArticleen_US

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