The observation of HII regions around dzeta OPH and other O-B stars.
Abstract
A Fabry-Perot spectrometer was used to measure the emission intensities in H-beta near Zeta Oph, Alpha Vir, Alpha Cam, and HD 188209. The spectrometer sensitivity is 0.2 rayleighs, the intensity measurement accuracy is 20 percent. Ionization zone boundaries are determined for Zeta Oph and Alpha Vir; the angular diameters of both regions are about 15 deg. The contour of the H II region near Zeta Oph on the level of the double background in the southwest does not close; instead, it expands again and incorporates the region associated with the B-association II Sco.
- Publication:
-
Pisma v Astronomicheskii Zhurnal
- Pub Date:
- January 1988
- Bibcode:
- 1988PAZh...14...60S
- Keywords:
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- B Stars;
- H Ii Regions;
- O Stars;
- Stellar Radiation;
- Astronomical Spectroscopy;
- Fabry-Perot Spectrometers;
- Spectral Sensitivity;
- Astrophysics