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dc.contributorEötvös Loránd University Budapest, Department of Astronomy
dc.contributorArmagh Observatory and Planetarium, College Hill, Armagh
dc.contributor.authorJoo, Andras Peter
dc.contributor.authorEden, David
dc.contributor.authorTóth, L. Viktor
dc.date.accessioned2024-10-02T19:40:50Z
dc.date.available2024-10-02T19:40:50Z
dc.date.issued2024-08-01T00:00:00Z
dc.identifier.other2024IAUGA..32P2397J
dc.identifier.other-
dc.identifier.urihttp://hdl.handle.net/20.500.14302/2126
dc.description.abstractThe Planck compact source catalogue provides excellent samples for studying the earliest phases of star formation. Covering all galactic longitudes and latitudes they can give an overview of how star formation varies throughout the Milky Way, enabling a better insight into star formation out of the Galactic plane, where our current understanding is restricted mostly to nearby clouds. We examined the 200 brightest Planck compact sources visible from the northern hemisphere using observations from the James Clerk Maxwell Telescope's SCUBA2 bolometer array. Its high resolution revealed diverse, mostly filamentary structures, and allowed the extraction of point sources from the maps. We classified more than 1500 of these point sources and compiled a catalogue with their positions, sizes, and physical parameters. In our statistical analysis, we investigate properties of star-forming regions at different latitudes, aiming to better understand the flow of interstellar matter in the Galaxy and thus refine our latest view of the Milky Way.
dc.publisherIAU General Assembly
dc.titlePre- and protostellar cores in the 200 brightest Planck compact sources
dc.typeabstract
dc.source.journalIAUGA
dc.source.journalIAUGA..32
dc.identifier.bibcode2024IAUGA..32P2397J


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