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...
Spremljeno u:
| Izdano u: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Glavni autori: | , , , |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2003
|
| Teme: | |
| Online pristup: | https://www.redalyc.org/articulo.oa?id=57139103 |
| Oznake: |
Bez oznaka, Budi prvi tko označuje ovaj zapis!
|