... Due to strong weakening (about 6 mag) of a photospheric spectrum of the star we can see the spectrum of the nebulae (emission in HI, NII), the spectrum of cold envelope (emission bands of the molecule C2, atomic ...
... Discovery of the acceleration in the wind emission lines of CI Cam. ... The centroid velocities of the following emission lines were measured: FeII (5 lines ... velocities of narrow telluric [O I] emission line and two components of interstellar ...
... about 6 mag) of a photospheric spectrum of the star we can see the spectrum of the nebulae (emission in HI, NII), the spectrum of cold envelope (emission bands of the molecule C2, atomic emissions) and the high velocity spectrum of the NaI doublet ...
... Velocity profiles of the HI emission in the whole of this region may be clearly divided into two parts: rather narrow picks near zero velocity and the very broad emission which is obviously arised from far (mainly - back) sidelobes of our antenna. ...
... a regular Z(S)-shaped pattern of the emission filaments appears on images . ... have revealed a double-component structure of the [OIII] emission line profiles ... 3 was observed 15 Nov. 1996 in the [OIII]5007 emission line with IPCS as detector ...
... The intensity of line emission of neutral hydrogen (HI) is proportional to concentration of gas and is inverse proportional its temperature.Therefore the reduction of intensity emission of HI in dust clouds could not be interpeted simple. ...
... presented here contain 21 cm HI emission contours around 98 Super Nova Remnants (SNR ... diameters more than 10' and morphological type in continuum emission - S (shell ...
... Next: Emission molecular bands Up: Optical spectrum of IRAS04296 Previous: Optical ... of the line (see Fig. 1 ), molecular emission bands and very strong absorption lines ...