Physical conditions in CaFe interstellar clouds

Preprint English OPEN
Gnacinski, P.; Krogulec, M.;

Interstellar clouds that exhibit strong Ca I and Fe I lines were called CaFe clouds. The ionisation equilibrium equations were used to model the column densities of Ca II, Ca I, K I, Na I, Fe I and Ti II in CaFe clouds. The chemical composition of CaFe clouds is that of... View more
  • References (20)
    20 references, page 1 of 2

    Badnell N.R., 2006, ApJSS, 167, 334

    Bagnulo et al., 2003, Messenger, 114, 10

    Black J.H., van Dishoeck E.F., 1991, ApJ, 369, L9

    Bondar A., Kozak M., Gnacin´ski P., Galazutdinov G. A., Beletsky Y., Krełowski J., 2007, MNRAS, 378 , 893

    de Boer K.S., Koppenaal K., Pottasch S.R., 1973, A&A, 28, 145

    Danks A.C., Federman S.R., Lambert D.L., 1984, A&A, 130, 62

    Federman S.R., 1982, ApJ, 257, 125

    Hunter I., Smoker J.V., Keenan F.P., Ledoux C., Jehin E., Cabanac R., Melo C., Bagnulo S., 2006, MNRAS, 367, 1478

    Gnacin´ski P., Krogulec M., 2006, Acta Astron., 56 , 373

    Gnacin´ski P., Krogulec M., Krełowski J., 2007, Proceedings of the conference ”Molecules in Space and Laboratory”, Paris 14-18 May 2007

  • Metrics
Share - Bookmark