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Lithium in giant Star 850 in stellar cluster Be21
FEROS obtained two spectra (each of 90 min exposure) of S50, both showing this strong Lithium line and thus proving that it cannot have been caused by an instrumental effect. These spectra also illustrate the great amount of information that may be obtained in each exposure with FEROS - the shown spectral interval is just 1/280 of the total range recorded. The (visual) magnitude of S50 is 15.6, i.e., about 7,000 times fainter than what can be seen with the unaided eye.
Crédito:ESO
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Identificador: | eso9905b |
Tipo: | Mapa |
Fecha de publicación: | 2 de Febrero de 1999 |
Noticias relacionadas: | eso9905 |
Tamaño: | 2936 x 3008 px |