SIMBAD references

1994A&A...285..535M - Astronomy and Astrophysics, volume 285535-540 (1994/5-2)

Studies of early-type variable stars XII. Spectroscopic orbit and absolute parameters of AT Pegasi.

MAXTED P.F.L., HILL G. and HILDITCH R.W.

Abstract (from CDS):

A new spectroscopic orbit is presented for the Algol system AT Peg (HD 210892, P=1.146 days, α(2000.0)=22h13.4m, δ=+8deg25.5', A4V+G). We find : mp sin 3i=2.04±0.06M☉, ms sin 3i=0.96±0.025M☉, (ap+as)sin i=4.62 ±0.06 x 106km, mp/ms=2.115±0.04. This is the first direct measure of the mass ratio for this system. The new mass ratio is used to solve the single colour light curve of Cristaldi & Walter (1963). We find the following absolute parameters: mp=2.22±0.065 M☉, ms=1.05±0.025M☉, <Rp ≥1.86±0.025R☉, <Rs ≥2.15± 0.03R , <Tp ≥ 8400±100K, < Ts ≥4900±200 K. The spectral type of the primary was established from a spectrum of the primary reconstructed from the spectroscopic data set using tomography. AT Peg is slightly reddened (E(B-V)=0.03±0.03) at a distance of 360±20parsecs.

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Journal keyword(s): stars: binaries: eclipsing - techniques: image processing - stars: individual: AT Peg - stars: fundamental parameters

Simbad objects: 3

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