Carbon stars in the X-shooter Spectral Library

التفاصيل البيبلوغرافية
العنوان: Carbon stars in the X-shooter Spectral Library
المؤلفون: Gonneau, A., Lançon, A., Trager, S. C., Aringer, B., Lyubenova, M., Nowotny, W., Peletier, R. F., Prugniel, P., Chen, Y. -P., Dries, M., Choudhury, O. S., Falcón-Barroso, J., Koleva, M., Meneses-Goytia, S., Sánchez-Blázquez, P., Vazdekis, A.
المصدر: A&A 589, A36 (2016)
سنة النشر: 2016
المجموعة: Astrophysics
مصطلحات موضوعية: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies
الوصف: We provide a new collection of spectra of 35 carbon stars obtained with the ESO/VLT X-shooter instrument as part of the X-shooter Spectral Library project. The spectra extend from 0.3$\mu$m to 2.4$\mu$m with a resolving power above $\sim$ 8000. The sample contains stars with a broad range of (J-K) color and pulsation properties located in the Milky Way and the Magellanic Clouds. We show that the distribution of spectral properties of carbon stars at a given (J-K) color becomes bimodal (in our sample) when (J-K) is larger than about 1.5. We describe the two families of spectra that emerge, characterized by the presence or absence of the absorption feature at 1.53$\mu$m, generally associated with HCN and C$_2$H$_2$. This feature appears essentially only in large-amplitude variables, though not in all observations. Associated spectral signatures that we interpret as the result of veiling by circumstellar matter, indicate that the 1.53$\mu$m feature might point to episodes of dust production in carbon-rich Miras.
Comment: 29 pages, 21 figures, 9 tables, Accepted for publication in A&A
نوع الوثيقة: Working Paper
DOI: 10.1051/0004-6361/201526292
URL الوصول: http://arxiv.org/abs/1602.00887
رقم الأكسشن: edsarx.1602.00887
قاعدة البيانات: arXiv
الوصف
DOI:10.1051/0004-6361/201526292