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| Format: | Artículo científico |
| Language: | en |
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Universidad Nacional Autónoma de México
2017
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| Online Access: | https://www.redalyc.org/articulo.oa?id=57153206021 |
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| _version_ | 1866586228169637888 |
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| author | S. Gaudenzi |
| author_facet | S. Gaudenzi |
| contents | INFRARED CHARACTERISTICS OF THE BIS CATALOG OBJECTS S. Gaudenzi R. Nesci C. Rossi S. Sclavi K. S. Gigoyan A. M. Mickaelian Física, Astronomía y Matemáticas stars: late type stars: infrared sources stars: variables: general We studied several color-color infrared diagrams of the 276 late type stars of the BIS catalog. For 95 of these stars we derived spectral classification from our slit spectroscopy. From the 2MASS color diagram we concluded that none of the sample stars is a dwarf. The WISE 3.4-12 vs 12-22 plot is the best to discriminate the variability type (Mira, irregular and not-variable), as well as carbon stars. IRAS colors are less useful due to the poor quality of the data for most of the BIS stars. Mixed plots involving 2MASS, AKARI and WISE were also explored: the 2MASSAKARI J-[S09] vs [S09]-[L18] plot is efficient to discriminate carbon and Mira stars. From the color plots and our spectroscopy we can statistically predict that in the whole BIS catalog no other dusty carbon star is present, while a few Miras and CH or R carbon stars could be discovered. Only about 15% of the BIS stars are of early M type. 2017 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57153206021 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.53 |
| format | Artículo científico |
| id | redalyc_57153206021 |
| language | en |
| publishDate | 2017 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | INFRARED CHARACTERISTICS OF THE BIS CATALOG OBJECTS S. Gaudenzi Física, Astronomía y Matemáticas stars: late type stars: infrared sources stars: variables: general INFRARED CHARACTERISTICS OF THE BIS CATALOG OBJECTS S. Gaudenzi R. Nesci C. Rossi S. Sclavi K. S. Gigoyan A. M. Mickaelian Física, Astronomía y Matemáticas stars: late type stars: infrared sources stars: variables: general We studied several color-color infrared diagrams of the 276 late type stars of the BIS catalog. For 95 of these stars we derived spectral classification from our slit spectroscopy. From the 2MASS color diagram we concluded that none of the sample stars is a dwarf. The WISE 3.4-12 vs 12-22 plot is the best to discriminate the variability type (Mira, irregular and not-variable), as well as carbon stars. IRAS colors are less useful due to the poor quality of the data for most of the BIS stars. Mixed plots involving 2MASS, AKARI and WISE were also explored: the 2MASSAKARI J-[S09] vs [S09]-[L18] plot is efficient to discriminate carbon and Mira stars. From the color plots and our spectroscopy we can statistically predict that in the whole BIS catalog no other dusty carbon star is present, while a few Miras and CH or R carbon stars could be discovered. Only about 15% of the BIS stars are of early M type. 2017 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57153206021 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.2 Vol.53 |
| title | INFRARED CHARACTERISTICS OF THE BIS CATALOG OBJECTS |
| topic | Física, Astronomía y Matemáticas stars: late type stars: infrared sources stars: variables: general |
| url | https://www.redalyc.org/articulo.oa?id=57153206021 |