The Optical and Near-Infrared Counterpart of IRAS 18476+2054
We present here, for the first time, an optical and near-infrared (NIR) identification for the previously unstudied IRAS PSC source 18476+2054. Direct imagingin BVRICiJKs and optical spectroscopy were obtained. The optical counterpart isidentified as a variable star of Mira class M7 or later giant...
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| Vydáno v: | Revista Mexicana de Astronomía y Astrofísica |
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| Hlavní autoři: | , , , |
| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Universidad Nacional Autónoma de México
2003
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| Témata: | |
| On-line přístup: | https://www.redalyc.org/articulo.oa?id=57139103 |
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