The Use of Near Infrared Spectroscopy to Reclassify HR:8881

Bibcode
1994MNRAS.266..678H
Hammersley, P. L.; Kidger, M. R.; Mampaso, A.
Referencia bibliográfica

Monthly Notices of the Royal Astronomical Society, Vol. 266, NO. 3/FEB1, P. 678, 1994

Fecha de publicación:
2
1994
Revista
Monthly Notices of the Royal Astronomical Society
Número de autores
3
Número de autores del IAC
1
Número de citas
2
Número de citas referidas
2
Descripción
We demonstrate that near-infrared CVF spectrometry can be used to determine accurately the spectral type and luminosity class of K- and M-type stars. As an example, we show that the spectral type and luminosity class of the star HR 8881 given in the fourth edition of the Bright Star Catalogue are in error. HR 8881 is an M giant, probably in the range M2-3III, and not a type-K dwarf as listed.
Tipo
Con árbitro
Técnicas

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