Multi-epoch <i>L</i>-band Spectroscopy of the Be Star μ Centauri Prior to Outburst

With the aim of contributing to the understanding of the disk formation process in Be stars, we pursued a one-year spectroscopic observing campaign of the Be star μ Centauri in the <i>L</i>-band, using VLT/ISAAC. We present the nine near-IR spectra we obtained in an epoch of relative pho...

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Detalles Bibliográficos
Autores principales:	Aguayo, G., Mennickent, R. E., Granada, Anahí, Otero, S.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2018
Materias:	Astronomía circumstellar matter infrared: stars stars: emission-line, Be stars: mass-loss
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93705 https://iopscience.iop.org/article/10.3847/1538-3881/aad5db https://ri.conicet.gov.ar/handle/11336/82431
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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