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...
Gorde:
| Argitaratua izan da: | Revista Mexicana de Astronomía y Astrofísica |
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| Egile Nagusiak: | , , , , , , |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
Universidad Nacional Autónoma de México
2010
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| Gaiak: | |
| Sarrera elektronikoa: | https://www.redalyc.org/articulo.oa?id=57115706033 |
| Etiketak: |
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