VBLUW photometry of solar-type stars

Details VBLUW photometry of solar-type stars VBLUW photometry of solar-type stars

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...160..392g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 160, no. 2, May 1986, p. 392-397.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Catalogs, Late Stars, Stellar Spectrophotometry, Visual Photometry, Abundance, Stellar Color, Stellar Gravitation, Stellar Temperature

Scientific paper

VBLUW photometric observations of 35 solar-type stars are presented and
discussed in terms of abundance, Teff and gravity (log g).
Using the empirical transformation between the VBLUW and UBV systems,
for four stars being very similar to the sun the authors derive (B-V) =
0.656±0.011.

Affiliated with

Also associated with

No associations

Rating

VBLUW photometry of solar-type stars 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 VBLUW photometry of solar-type stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VBLUW photometry of solar-type stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1772216