THE 2008+ OUTBURST OF THE BE STAR 28 CMA
The precursor phase of the outburst started in October 2008 was intensively monitored by photometry, highresolution optical and near-IR spectroscopy and interferometry. Contrary to the expected monotonic outburst a long precursor phase with cyclic smaller outbursts was observed. A more distant part...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2010
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57115706033 |
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