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dc.date.accessioned 2022-09-19T12:53:21Z
dc.date.available 2022-09-19T12:53:21Z
dc.date.issued 1988
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/142271
dc.description.abstract We present spectrograms of the central stars of the planetary nebulae IC 3568, IC 4593, NGC 6826, NGC 6543 and NGC 6572, obtained at La Palma, using the Intermedíate Dispersión Spectrograph and a CCD detectors attached to the Cassegrain focus of the 2.5m Isaac Newton telescope. We obtained a spectral resolution of 0,6 Angstroms. We have searched for spectral and radial velocity variations and we have made, whenever possible, a quantitative spectroscopic analysis of the photospheric line profiles. Besides, we have found that the nebular He II emission at 4686 Angstroms in the spectrum of NGC 6572 is stronger than 20 years ago. This may imply an increase in the effective temperature of the central star. en
dc.language es es
dc.subject Galaxia es
dc.title Observations of central stars of planetary nebulae from La Palma en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Méndez, R.H. es
sedici.creator.person Herrero, A. es
sedici.creator.person Manchado, A. 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. 34 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) es


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