HRI observations of PMS stars in NGC 2264

Astronomy and Astrophysics

Volumn 355, Issue 2, 2000, Pages 651-667

  Flaccomio, E ^a   Micela, G ^b   Sciortino, S ^b   Damiani, F ^b   Favata, F ^c   Harnden Jr , F R ^d   Schachter, J ^d  

^a UNIVERSITY OF PALERMO   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

^c EUROPEAN SPACE AGENCY   (Netherlands)

^d HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Galaxy: open clusters and associations: individual: NGC 2264; Mass function; Stars: coronae; Stars: formation; Stars: luminosity function; Stars: pre main sequence; X rays: stars

Indexed keywords

EID: 0000813211     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (19)

1. Alcalá J.M., Krautter J.,Covino E., et al., 1997, A&A 319, 184
2. Bessel M.S., 1990, PASP 102, 1181
3. Bessel M.S., Stringfellow G.S., 1993, ARA&A 31, 433
4. Casanova S., Montmerle T., Feigelson E.D., André P., 1995, ApJ 439, 752
5. Code A.D., Davis J., Bless R. C., Hanbury Brown R., 1976, ApJ 203, 417
6. Cousin A.W.J., 1980, South African Astronomical Observatory Circular 1, 234
7. Damiani F., Micela G., 1995, ApJ 446, 341
8. Damiani F., Maggio A., Micela G., Sciortino S., 1997a, ApJ 483, 350
9. Damiani F., Maggio A., Micela G., Sciortino S., 1997b, ApJ 483, 370
10. D'Antona F., Mazzitelli I., 1998, In: Micela G., Pallavicini R., Sciortino S. (eds.) Mem. Soc. Astron. Ital. Vol. 68. No. 4
11. David L.P., Harnden F.R. Jr., Kearns K.E., Zombeck M.V., 1997, The ROSAT High Resolution Imager (HRI) Calibration Report
12. Feigelson E.D., Kriss G.A., 1981, ApJ 248, L35
13. Simon T., Cash W., Snow T.P. Jr., 1985, ApJ 293, 542
14. Snow T.P. Jr., Cash W., Grady C.A., 1981, ApJ 19, L244
15. Sung H., Bessell M.S., Lee S.-W., 1997, AJ 114, 2644
16. Vasilevskis S., Sanders W.L., Balz A.G.A.J., 1965, AJ 70, 797
17. Walter F.M., Kuhi L.V., 1981, ApJ 250, 254
18. Walker M.F., 1956, ApJS 2, 365
19. Zombeck M.V., Conroy M., Harnden F.R. Jr., et al., 1990, Proceedings of the SPIE Conference on EUV, X-Ray and Gamma-Ray Instrumentation for Astronomy, 1344, 267