Spectro- and UBV photometry of the anomalous planetary nebula FG Sagittae, 1968-77

Details Spectro- and UBV photometry of the anomalous planetary nebula FG Sagittae, 1968-77 Spectro- and UBV photometry of the anomalous planetary nebula FG Sagittae, 1968-77

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..389s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, June-July 1979, p. 389-393.

Astronomy and Astrophysics

Astronomy

12

Astronomical Photometry, Planetary Nebulae, Stellar Spectrophotometry, Ubv Spectra, Variable Stars, Continuous Spectra, Gas Temperature, Long Term Effects, Optical Thickness, Rates (Per Time), Stellar Envelopes

Scientific paper

Continuum scans of FG Sge taken over the last ten years are compared
with a grid of scans of the continua of MK standard stars. The effective
temperature of the optically thick shell is determined from the
observations, and a mean cooling rate of about 310 K per year is
established.

Affiliated with

Also associated with

No associations

Rating

Spectro- and UBV photometry of the anomalous planetary nebula FG Sagittae, 1968-77 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 Spectro- and UBV photometry of the anomalous planetary nebula FG Sagittae, 1968-77, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectro- and UBV photometry of the anomalous planetary nebula FG Sagittae, 1968-77 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1778687