An expanding high velocity hi cloud probably ejected from the galactic nucleus

dc.creatorMirabel Miquele, Igor Félix
dc.creatorFranco, M. L.
dc.date1976
dc.date2022-08-05T19:22:04Z
dc.date.accessioned2023-07-15T04:52:30Z
dc.date.available2023-07-15T04:52:30Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/140070
dc.identifierissn:0004-640x
dc.identifierissn:1572-946x
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7471215
dc.descriptionAn object located approximately atl=8°,b=−4° with a mean radial velocity of −212.3 km s−1 has been observed in the 21 cm neutral hydrogen line. The mean weighted velocity dispersion is 11.2 km s−1 and the total mass is estimated to be 190R2 (kpc) solar masses. We discuss possible interpretations of the origin and nature of this object. The most likely interpretation is that we observe an expanding object which has been ejected from the galactic nucleus.
dc.descriptionInstituto Argentino de Radioastronomía
dc.formatapplication/pdf
dc.format483-494
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by/4.0/
dc.rightsCreative Commons Attribution 4.0 International (CC BY 4.0)
dc.subjectCiencias Exactas
dc.subjectAstronomía
dc.subjectHydrogen
dc.subjectTotal Mass
dc.subjectHigh Velocity
dc.subjectRadial Velocity
dc.subjectVelocity Dispersion
dc.titleAn expanding high velocity hi cloud probably ejected from the galactic nucleus
dc.typeArticulo
dc.typeArticulo


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