... cloud diameters, that is found from molecular clouds, in the case of HI clouds is ... clouds have systematic velocity gradient across cloud disks that is may be due to ...
... The international conference . "Absorption Spectra of Translucent Interstellar Clouds: . Observers meet Experimentalists" . ... Purposes and tasks of the conference. Absorption spectra of translucent interstellar clouds are complex and involve: . ...
... molecules (identified and DIB carriers) differ from cloud to cloud due to different physical processes which govern their ... Also DIB profiles vary from cloud to cloud - this fact strongly supports a molecular origin of these, still unidentified ...
... The neutral hydrogen in dust cloud . (1964) . ... reduction of intensity emission of HI in dust clouds could not be interpeted simple ... frequencies and coordinates of the dense dust cloud which covered the most part of ...
... The compression of the cloud of gas in star forming . region Sagittarius B2 . ... have allowed us to create the dynamic model of the cloud of gas, around this object ...
... Spectra of the various characteristics of interstellar clouds . (1989) . ... on RATAN-600 it is revealed 98 interstellar HI clouds with the sizes from 0.2 up to ... interstellar matter the process of coalescence in cloud-cloud collisins predominates ...
... These data show that in the middle mass range the process of coalescence in cloud-cloud collisions predominates but the clouds with low masses are evaporated probably due to very hot ISM component. ...
... The distribution of the axes of rotation of clouds in space is random, which leads to the conclusion that the collision of clouds is the main source of their rotation. ...
... Clouds of gas between spiral arms . (1978) . ... centres of Galaxy 11 - 12 kpc 81 HI clouds are found and their parameters (figure 1 ... It has appeared, that the clouds make the "wide" component of gas and are ...