... The radial velocity curve of the HeII emission (middle) . ... FeII emissions forming in the stellar wind have rectangular profile of 1.2A width ... us note that the intensity of HeII emission increased in the peak of the outburst by ...
... Velocity field . Mkn 1157 was observed 1 Sep. 2002 in the Ha emission line. ... was observed September, 23 2000 in the Ha emission line, Texp=32x120 sec, seeing 2.5 ...
... medium of our Galaxy using its line emission in radio domain with the help of the ... The observation of interstar gas emission with a large region all over the sky. ...
... loss of information is due to the overestimation of the scattered light in the region of and to the broad emission lines and ... In Table 1 are given only emission lines. ...
... region, it is well seen that the emission component of the shell decreases rapidly ... the analysis, as their profiles in CI Cam were distorted by emissions least of all ...
... Angular structure of the interstellar HI emission at 21 cm was investigated on the ... Angular power spectrum of interstellar HI emission was computed with standard FFT ...
... The apparent emission in the strong,stellar helium line is a result of division to eliminate telluric lines by a standard star with stellar helium in absorption. ...