2013AJ....145...38P


Query : 2013AJ....145...38P

2013AJ....145...38P - Astron. J., 145, 38 (2013/February-0)

On the six-year period in the radial velocity of Antares A.

PUGH T. and GRAY D.F.

Abstract (from CDS):

We examine the century-long historical data and compare it with our new radial-velocity measurements to determine an improved period. We find a period of 2167±5 days (5.93±0.01 years). Both orbital motion and pulsation are considered as possible causes of the velocity variation. Temperature variations we deduce from line-depth ratios support the pulsation hypothesis. A temperature minimum occurs in 2009, 70 days after the radial-velocity minimum. We deduce a radius change of 19%±4% from an integration of the radial-velocity curve and predict a visual magnitude variation ∼0.2 from the radius and temperature variation.

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Journal keyword(s): binaries: spectroscopic - stars: individual: α Sco A - stars: oscillations, including pulsations - stars: variables: general - techniques: radial velocities - techniques: spectroscopic

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 * alf Ori s*r 05 55 10.30536 +07 24 25.4304 4.38 2.27 0.42 -1.17 -2.45 M1-M2Ia-Iab 1789 0
2 * alf Sco B Em* 16 29 24.20 -26 25 51.0   5.0 5.2     B2.5V 119 0
3 * alf Sco s*r 16 29 24.45970 -26 25 55.2094 4.08 2.75 0.91 -0.64 -1.87 M1.5Iab+B2Vn 786 0
4 * alf Her ** 17 14 38.85818 +14 23 25.2262           M5Ib-II+G5III+F2V: 209 0

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