The object R 136 and its nearer surroundings in the gas nebula 30 Doradus

Details The object R 136 and its nearer surroundings in the gas nebula 30 Doradus The object R 136 and its nearer surroundings in the gas nebula 30 Doradus

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....56..245f&link_type=abstract

Astronomy and Astrophysics, vol. 56, no. 1-2, Apr. 1977, p. 245-250. In German.

Astronomy and Astrophysics

Astrophysics

8

Galactic Nuclei, Hydrogen Clouds, Magellanic Clouds, Nebulae, Stellar Spectrophotometry, Ubv Spectra, Electrophotometry, Emission Spectra, H Alpha Line, Hot Stars, Line Spectra, Luminous Intensity, O Stars, Spectral Line Width, Telescopes

Scientific paper

By photoelectric UBV photometry, photographs in UVR, and spectrophotometric measurements the extraordinary nature of R 136, central star in the 30 Doradus nebula, is demonstrated. Some evidence is presented for the variation of intensity and of spectral lines on time scales of 2-3 days. An upper limit of 0.12 is given for the forbidden N II/H-alpha intensity ratio of this object. The emitted energy in H-alpha is 3 by 10 to the 36th power erg/s, and the mean H-alpha line halfwidth 6 A.

Affiliated with

Also associated with

No associations

Rating

The object R 136 and its nearer surroundings in the gas nebula 30 Doradus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The object R 136 and its nearer surroundings in the gas nebula 30 Doradus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The object R 136 and its nearer surroundings in the gas nebula 30 Doradus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1616377