Constraints on the origin of manganese from the composition of the sagittarius dwarf spheroidal galaxy and the Galactic bulge

Astrophysical Journal

Volumn 592, Issue 1 II, 2003, Pages

  McWilliam, Andrew ^a   Rich, R Michael ^b   Smecker Hane, Tammy A ^c  

^a CARNEGIE OBSERVATORIES   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Galaxies: dwarf; Galaxies: individual (Sagittarius dwarf spheroidal); Galaxy: bulge; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances

Indexed keywords

EID: 0041332878     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/377441     Document Type: Article

References (35)

1. Arnett, W. D. 1971, ApJ, 166, 153
2. Bonifacio, P., Hill, V., Molaro, P., Pasquini, L., Di Marcantonio, P., & Santin, P. 2000, A&A, 359, 663
3. Cunha, K., Smith, V. V., Suntzeff, N. B., Norris, J. E., DaCosta G. S., & Plez, B. 2002, AJ, 124, 379
4. Feltzing, S., & Gustafsson, B. 1998, A&AS, 129, 237 (FG98)
5. Gratton, R. G. 1989, A&A, 208, 171 (G89)
6. Grebel, E. K. 2000, in 33d ESLAB Symp., Star Formation from the Small to the Large Scale, ed. F. Favata, A. A. Kaas, & A. Wilson (ESA SP-445; Noordwijk: ESA), 87
7. Helfer, H. L., Wallerstein, G., & Greenstein, J. L. 1959, ApJ, 129, 700
8. Hinkle, K., Wallace, L., Valenti, J., & Harmer, D., eds. 2000, Visible and Near Infrared Atlas of the Arcturus Spectrum 3727-9300 Å (San Francisco: ASP)
9. Iben, I. G., & Tutukov, A. V. 1987, ApJ, 313, 727
10. Johnson, J. A. 2002, ApJS, 139, 219
11. _. 1997, in IAU Symp. 189, Fundamental Stellar Properties: The Interaction between Observation and Theory, ed. T. R. Bedding, A. J. Booth, & J. Davis (Dordrecht: Kluwer), 217
12. Mateo, M. 1998, ARA&A, 36, 435
13. Matteucci, M., Romano, D., & Molaro, P. 1999, A&A, 341, 458
14. McWilliam, A., Preston, G. W., Sneden, C., & Shectman, S. 1995, AJ, 109, 2736
15. McWilliam, A., & Rich, R. M. 1994, ApJS, 91, 749
16. McWilliam, A., & Rich, R. M. 1999, in Chemical Evolution from Zero to High Redshift, ed. J. R, Walsh & M. R. Rosa (Berlin: Springer), 73
17. Nissen, P. E., Chen, Y. Q., Schuster, W. J., & Zhao, G. 2000, A&A, 353, 722 (N00)
18. Nissen, P. E., & Schuster, W. J. 1997, A&A, 326, 751
19. Ortolani, S., et al. 1995, Nature, 377, 701
20. Prochaska, J. X., & McWilliam, A. 2000, ApJ, 537, L57 (PM00)
21. Prochaska, J. X., Naumov, S. O., Carney, B. W., McWilliam, A., & Wolfe, A. M. 2000, AJ, 120, 2513 (P00)
22. Reddy, B. E., Tomkin, J., Lambert, D. L., & Allende Prieto, C. 2003, MNRAS, 340, 304 (R03)
23. Rich, R. M. 1990, ApJ, 362, 604
24. Rich, R. M., & McWilliam, A. 2000, Proc. SPIE, 4005, 150
25. Searle, L., & Sargent, W. L. W. 1972, ApJ, 173, 25
26. Shetrone, M. D., Coté, P., & Sargent, W. L. W. 2001, ApJ, 548, 592
27. Smecker-Hane, T., & McWilliam, A. 2003, ApJ, submitted (SM03)
28. Smecker-Hane, T., & Wyse, R. F. G. 1992, AJ, 103, 1621
29. Sneden, C. 1973, ApJ, 184, 839
30. Tinsley, B. M. 1979, ApJ, 229, 1046
31. Tornambè, A., & Matteucci, F. 1986, MNRAS, 223, 69
32. Vogt, S. S., et al. 1994, Proc. SPIE, 2198, 362
33. Wallerstein, G. 1962, ApJS, 6, 407
34. Woosley, S. E., & Weaver, T. A. 1995, ApJS, 101, 181
35. Zoccali, M., et al. 2003, A&A, 399, 931