dc.creatorWeidmann, W. A.
dc.creatorGamen, Roberto Claudio
dc.date2010
dc.date2019-10-02T17:43:15Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/82539
dc.identifierissn:0004-6361
dc.descriptionContext. There are more than 3000 confirmed and probable known Galactic planetary nebulae (PNe), but central star spectroscopic information is available for only 13% of them. Aims. We undertook a spectroscopic survey of central stars of PNe at low resolution and compiled a large list of central stars for which information was dispersed in the literature. Methods. We observed 45 PNs using the 2.15 m telescope at Casleo, Argentina. Results. We present a catalogue of 492 confirmed and probable CSPN and provide a preliminary spectral classification for 45 central star of PNe. This revises previous values of the proportion of CSPN with atmospheres poor in hydrogen in at least 30% of cases and provide statistical information that allows us to infer the origin of H-poor stars.
dc.descriptionInstituto de Astrofísica de La Plata
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.languageen
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.subjectCiencias Astronómicas
dc.subjectplanetary nebulae: general
dc.subjectstars: evolution
dc.subjectsurveys
dc.titleCentral stars of planetary nebulae: New spectral classifications and catalogue
dc.typeArticulo
dc.typeArticulo


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