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- W1974643535 abstract "view Abstract Citations (27) References (26) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Superluminous giants in Magellanic Cloud clusters. Flower, P. J. Abstract The C-M diagram of the LMC blue, globular-like cluster NGC 1866 is known to exhibit a large number of yellow- and red-core helium-burning giants. Short exposure photographic plates taken with the CTIO 4-m Ritchey-Chretien camera provide an opportunity to study the stellar content of the central regions of this cluster. In and near the core of NGC 1866, 11 superluminous giants (SLGs), apparently similar to those found in other LMC blue, globular-like clusters, have been identified. These stars lie more than 0.5 mag above the core helium-burning giants. It is proposed that SLGs are protoplanetary nebulae, i.e., stars that, having ejected their envelopes as luminous red giants, are crossing the C-M diagram toward becoming central star planetary nebulae. Publication: The Astrophysical Journal Pub Date: October 1981 DOI: 10.1086/183647 Bibcode: 1981ApJ...249L..11F Keywords: Giant Stars; Late Stars; Magellanic Clouds; Planetary Nebulae; Star Clusters; Stellar Luminosity; Globular Clusters; Star Distribution; Stellar Evolution; Stellar Magnitude; Astronomy full text sources ADS | data products SIMBAD (3)" @default.
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- W1974643535 date "1981-10-01" @default.
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- W1974643535 title "Superluminous giants in Magellanic Cloud clusters" @default.
- W1974643535 doi "https://doi.org/10.1086/183647" @default.
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