Why observe AGB stars at mid-IR wavelengths from Dome C?

EAS Publications Series

Volumn 33, Issue , 2008, Pages 297-300

  Guandalini, R ^a   Briguglio, R ^b  

^a UNIVERSITY OF PERUGIA   (Italy)

^b SAPIENZA UNIVERSITY OF ROME   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

DOMES;

AGB STARS; ASYMPTOTIC GIANT BRANCHES; IR WAVELENGTHS; LONG TIMES; STELLAR EVOLUTIONS;

STARS;

EID: 57149125841     PISSN: 16334760     EISSN: 16381963     Source Type: Book Series    
DOI: 10.1051/eas:0833044     Document Type: Conference Paper

References (6)

1. Busso, M., Gallino, R., & Wasserburg, G.J., 1999, ARA&A, 37, 239
2. Busso, M., Guandalini, R., Persi, P., Corcione, L., & Ferrari-Toniolo, M., 2007, AJ, 133, 2310
3. Guandalini, R., Busso, M., Ciprini, S., Silvestro, G., & Persi, P., 2006, A&A, 445, 1069
4. Guandalini, R., & Busso, M., 2007, in preparation
5. Maffei, P., & Tosti, G., 1999, Internai Report Univ. Perugia
6. Sedlmayr, E., 1994, Lecture Notes Phys., 428, 163