Skip to main content Accessibility help
×
Home

Cold HI Gas in the Chamaeleon I Dark Cloud Region

  • F. Sato (a1), J. B. Whiteoak (a2), R. E. Otrupcek (a2) and M. Shimizu (a3)

Abstract

We have detected a large cold HI cloud consisting of several fragments in the region south of the Chamaeleon I dark cloud. The cold HI cloud is shown to be a future site of star formation.

Copyright

References

Hide All
Baud, B. et al., 1984, Astrophys. J. Lett., 278, L53.
Hasegawa, T., Sato, F. and Fukui, Y., 1983, Astron. J., 88, 658.
Hyland, A. R., Jones, T. J. and Mitchell, R. M., 1982, Mon. Not. R. Astr. Soc., 201, 1095.
Knapp, G. R., 1974, Astron. J., 79, 527.
Matilla, K. et al., 1989, ESO Conf. and Workshop Proc. No. 33, Reinpuith, B. (ed), p. 53.
Sata, F., 1990, Astron. J., 99, 1897.
Sato, F., Whiteoak, J.B., Otrupcek, R. E. and Tokushige, T., 1991, this volume.
Schwartz, R. D., 1977, Astrophys. J. Suppl. Ser., 35, 161.
Troiseva, M. and Mattila, K., 1985, Astron. Astrophys., 153, 207.
Whittet, D.C.B., Kirrane, T. M., Kilkenny, D., Oates, A. P., Watson, F. G. and King, D. J., 1987, Mon. Not. R. Astr. Soc., 224, 497.

Metrics

Full text views

Total number of HTML views: 0
Total number of PDF views: 0 *
Loading metrics...

Abstract views

Total abstract views: 0 *
Loading metrics...

* Views captured on Cambridge Core between <date>. This data will be updated every 24 hours.

Usage data cannot currently be displayed