On the Origin of a Sample of Suspected CH Stars in the Large Magellanic Cloud

We present (R— I)KC photometry based on optical spectrophotometry, and JHK photometry for the carbon stars suspected of being CH stars discovered by Hartwick and Cowley (1988) in the field of the LMC. These carbon stars are shown to be more luminous than the red giant branch tip of the Galactic Popu...

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Veröffentlicht in:	Publications of the Astronomical Society of the Pacific 1993-04, Vol.105 (686), p.350-359
Hauptverfasser:	Suntzeff, Nicholas B., Phillips, M. M., Elias, J. H., Cowley, A. P., Hartwick, F. D. A., Bouchet, P.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical magnitude Astronomical photometry Astronomy Asymptotic giant branch stars Carbon stars CH stars Earth, ocean, space Exact sciences and technology Population II stars Pre-main sequence objects, young stellar objects (yso's) and protostars (t tauri stars, orion population, herbig-haro objects, bok globules, bipolar outflows, cometary nebulae, etc.) Stars Stellar populations Stellar spectra Velocity
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