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dc.date.accessioned 2020-05-07T12:03:28Z
dc.date.available 2020-05-07T12:03:28Z
dc.date.issued 1969
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/95207
dc.description.abstract A series of lunar occultations of the galactic center region is being observed with the 140 foot telescope at Green Bank, West Virginia. In line observations, main interest lies in the fine structure of the absorbing clouds of OH or HI in front of the continuum sources near the center. The +40 km/sec component of the OH absorption spectrum is found to originate in a cloud of dimensions 3' x 5', which appears to rotate as a uniform body. Internal structure has been detected in the -130 km/sec component of the order of 30” . The results for the 1665 and 1667 MHz lines are significantly different. This paper has now been published in Astrophysical Letters, 2 , 195 - 200 (1968). es
dc.language es es
dc.subject Galaxias es
dc.title Observations of lunar occultations of the galactic center region in the OH and hydrogen lines en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Kerr, F. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 14 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)