... IFP produced by Queensgate Instruments Inc.) Interferometer Fabry Perot is a powerful device for investigation of the extended emission objects. ...
... We present the results of computation of linear diameter, density and HI mass spectra for about 5000 HI clouds, which were found by their emission at 21 cm with RATAN-600 radio telescope in the region of 180 degree -3 is not a power form, but has a ...
... Bond (ATel 966) reported that the blue emission lines of [FeII] continue to be strong, and very strong emission of H-alpha is detected in his October 12, November 29, and December 13, 2006 spectra. ...
... of the chemical evolution of Galaxy (galaxies) IS gas Observational manifestations: absorption lines and bands ( clouds); emission lines (HII regions, hot gas) IS dust Observational manifestations: IS extinction and polarization ( clouds); e scattered ...
... emission in the vicinity of the Milky Way consists of the following: a bright band ... emission from a truly "intermediate" component of the background radio emission of ...
... profiles with wide emission and narrow absorption not confirmed because such a ... the white dwarf were determined using HeII 4686 emission Kwd = 230 km/s = 51 km/s e ...
... Set images of ring picture from the reference emission line of He-Ne-Ar lamp need ... corresponding to a relatively shift the calibration emission line's center in NEON ... Shape of the emission line is a Airy profile really, but it is approximated as ...