caa a22 4500 469076585 CHVBK 20180323132936.0 cr unu---uuuuu 170328e19921101xx s 000 0 eng 10.1007/BF02506694 doi (NATIONALLICENCE)springer-10.1007/BF02506694 Molinari S. Istituto di Fisica Spazio Interplanetario, CNR, C.P. 27, 00044, Frascati, Italia aut Near-infrared variability ( (1 ÷ 10) μm ) of Herbig-Haro exciting sources [Elektronische Daten] [S. Molinari] Summary: We present the preliminary results of a systematic study intended for monitoring the photometric variations in the near IR ((1 ÷ 10) μm), exhibited by young sources responsible of considerable mass loss traced by Herbig-Haro (HH) objects, which are condensation of matter excited by interaction between the stellar wind and the circumstellar environment. Comparing the observed spectral shape variations with those predicted by models, positive indications in favour of accretion phenomena occurring in disks can be derived. Società Italiana di Fisica, 1992 98.70.Lt nationallicence IR Sources nationallicence 97.10 nationallicence Stellar characteristics and properties nationallicence Il Nuovo Cimento C Società Italiana di Fisica 15/6(1992-11-01), 1033-1038 0390-5551 15:6<1033 1992 15 11543 https://doi.org/10.1007/BF02506694 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/BF02506694 text/html Onlinezugriff via DOI NATIONALLICENCE 100 1- Molinari S. Istituto di Fisica Spazio Interplanetario, CNR, C.P. 27, 00044, Frascati, Italia aut NATIONALLICENCE 773 0- Il Nuovo Cimento C Società Italiana di Fisica 15/6(1992-11-01), 1033-1038 0390-5551 15:6<1033 1992 15 11543 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer