NEAR-INFRARED VARIABILITY ((1-DIVIDED-BY-10) MU-M) OF HERBIG-HARO EXCITING SOURCES

Authors
MOLINARI S
Citation
S. Molinari, NEAR-INFRARED VARIABILITY ((1-DIVIDED-BY-10) MU-M) OF HERBIG-HARO EXCITING SOURCES, Nuovo cimento della Societa italiana di fisica. C, Geophysics and space physics, 15(6), 1992, pp. 1033-1038
Citations number
NO
Categorie Soggetti
Geosciences, Interdisciplinary","Astronomy & Astrophysics
Journal title
Nuovo cimento della Societa italiana di fisica. C, Geophysics and space physics → ACNP
ISSN journal
11241896
Volume
15
Issue
6
Year of publication
1992
Pages
1033 - 1038
Database
ISI
SICI code
1124-1896(1992)15:6<1033:NV
Abstract
We present the preliminary results of a systematic study intended for monitoring the photometric variations in the near IR ((1 divided-by 10 ) mum), exhibited by young sources responsible of considerable mass lo ss traced by Herbig-Haro (HH) objects, which are condensation of matte r excited by interaction between the stellar wind and the circumstella r environment. Comparing the observed spectral shape variations with t hose predicted by models, positive indications in favour of accretion phenomena occurring in disks can be derived.