Fast photometry observations of the variable white dwarf GD 385

Details Fast photometry observations of the variable white dwarf GD 385 Fast photometry observations of the variable white dwarf GD 385

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...246..947v&link_type=abstract

Astrophysical Journal, Part 1, vol. 246, June 15, 1981, p. 947-950.

Astronomy and Astrophysics

Astrophysics

7

Stellar Oscillations, Stellar Spectrophotometry, Variable Stars, White Dwarf Stars, Fourier Analysis, Light Curve, Stellar Spectra

Scientific paper

The study of the variable GD 385 should be useful for understanding the mechanism at work in the variable white dwarfs. GD 385 behaves for long periods of time (months) like a typical, low-amplitude variable white dwarf. Suddenly, on a time scale of the order of days, the behavior of the variations may change. The light curve exhibits many significant frequencies or none at all. GD 385 evolved over two days from a state of low photometric activity (1979 June 25) to one of complex activity (1979 June 27). A description is presented of photometric observations of GD 385 which provide additional information on the sequence of events which occurred in 1979 June.

Affiliated with

Also associated with

No associations

Rating

Fast photometry observations of the variable white dwarf GD 385 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 Fast photometry observations of the variable white dwarf GD 385, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fast photometry observations of the variable white dwarf GD 385 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-991625