On coronal abundances derived with the SAX/LECS and ASCA/SIS detectors

Astronomy and Astrophysics

Volumn 326, Issue 3, 1997, Pages 1013-1022

  Favata, F ^a   Maggio, A ^b   Peres, G ^b   Sciortino, S ^b  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

Author keywords

Methods: Data analysis; Stars: Abundances; Stars: Late type; X rays: Stars

Indexed keywords

EID: 0000333621     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (11)

1. Ciaravella A., Maggio A., Peres G. 1997, A&A, 320, 945
2. Dotani T., Mitsuda K., Yamashita A. et al. 1996, ASCA Newsletter, 4
3. Drake S. A. 1996, in S. S. Holt, G. Sonneborn (eds.), Maryland conference on Cosmic Abundances, ASP, San Francisco, 215
4. Drake S. A., Singh K. P., White N. E., Simon T. 1994, ApJ, 436, L87
5. Eadie W., Drijard D., James F., Roos M., Sadoulet B. 1971, Statistical methods in experimental physics, 257, North-Holland
6. Jordan C. 1996, in S. Bowyer, R. F. Malina (eds.), Astrophysics in the extreme ultraviolet, IAU Colloquium 152, Kluwer, Dordrecht, p. 81
7. Maggio A., Favata F., Peres G., Sciortino S. 1997, A&A, submitted
8. Mewe R., Kaastra J. S., Liedahl D. A. 1995, Legacy, 6, 16
9. Parmar A. N., Martin D. D. E., Bavdaz M. et al. 1997, A&AS, 122, 309
10. Preibisch T. 1997, A&A, in press
11. Raymond J. C., Doyle J. G. 1981, ApJ, 247, 686