Negative detection of the four-hour periodicity of the central star of M1-2 (VV8)

Details Negative detection of the four-hour periodicity of the central star of M1-2 (VV8) Negative detection of the four-hour periodicity of the central star of M1-2 (VV8)

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..181y&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 1, Sept. 1984, p. 181-185.

Astronomy and Astrophysics

Astrophysics

3

Eclipsing Binary Stars, Periodic Variations, Planetary Nebulae, Spectrum Analysis, Stellar Spectrophotometry, Absorption Spectra, Balmer Series, Emission Spectra, Hot Stars, Radial Velocity, Stellar Magnitude, Supergiant Stars

Scientific paper

The four-hour (4.0002-hr) binary periodicity of the emission-line object
M1-2 (= VV8), claimed by Drummond (1980), is examined on the basis of
photometric and spectroscopic observations. However, neither positive
variation of the light nor of the radial velocity associated with that
period has been found.

Affiliated with

Also associated with

No associations

Rating

Negative detection of the four-hour periodicity of the central star of M1-2 (VV8) 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 Negative detection of the four-hour periodicity of the central star of M1-2 (VV8), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Negative detection of the four-hour periodicity of the central star of M1-2 (VV8) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1390053