dc.creatorDottori, Horacio Alberto
dc.date1994
dc.date2023-08-17T13:54:02Z
dc.date.accessioned2024-07-24T03:36:38Z
dc.date.available2024-07-24T03:36:38Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/156493
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9534670
dc.descriptionWe present observations of non-stellar emission objects in the field of the ionizing cluster NGC 3603. Spectroscopic and Photometric observations are used to analyze the physical properties of these intriguing objects. They are globules, about 0.1 pc in diameter, with high electronic density, which present emission characteristics of planetary nebulae. Their total brightness as well as the age of NGC 3603 and the large amount of objects detected argue against the PN hypothesis. We discuss the possibility of external ionization and conclude that they are objects partially ionized by the central ionizing cluster (PIGS) of NGC 3603.
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languagees
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectAstronomía
dc.subjectGalaxia
dc.titleNGC 3603 or the galaxy farm: forming stars or feeding pigs?
dc.typeArticulo
dc.typeComunicacion


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