1999A&A...350..859S


Query : 1999A&A...350..859S

1999A&A...350..859S - Astronomy and Astrophysics, volume 350859-864 (1999/10-3)

A comparative high-resolution spectroscopic study of the Hyades giants γ Tauri and ε Tauri.

SMITH G.

Abstract (from CDS):

Spectra of the Hyades K0 giants γ Tau and ε Tau in the regions 5852-5864Å and 6145-6176Å have been recorded at high resolution and with signal/noise in the range 150-250. A critical comparison reveals that, although nearly all lines in the observed regions have a similar depth, lines of ε Tau are broader by about 10% than those of γ Tau. An LTE analysis indicates that slightly higher turbulent broadening in ε Tau can account for the observed differences in line-width. Study of two particularly temperature sensitive features confirms earlier observations that the effective temperature of ε Tau is less than that of γ Tau and determines the temperature difference to be 80±20K.

Abstract Copyright: ∼

Journal keyword(s): stars: abundances - stars: fundamental parameters - stars: individual: γ Tau - stars: individual: ε Tau - stars: late-type

Simbad objects: 8

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Number of rows : 8
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 * eps Eri BY* 03 32 55.8444911587 -09 27 29.739493865 5.19 4.61 3.73 3.00 2.54 K2V 2073 1
2 * gam Tau ** 04 19 47.6039239005 +15 37 39.511385129 5.46 4.64 3.65 4.83   G9.5IIIabCN0.5 569 0
3 * eps Tau ** 04 28 37.0002551195 +19 10 49.563140930 5.42 4.54 3.53     G9.5IIICN0.5 628 1
4 Cl Melotte 25 OpC 04 30 27.4 +16 46 43           ~ 3309 0
5 * bet Gem PM* 07 45 18.94987 +28 01 34.3160 3.00 2.14 1.14 0.39 -0.11 K0IIIb 1150 2
6 * ksi Boo A PM* 14 51 23.3884659504 +19 06 01.619801424   5.40 4.675     G7Ve 564 0
7 * lam Peg PM* 22 46 31.8779099972 +23 33 56.361958743 5.93 5.00 3.93 3.16 2.66 G8IIIaCN0.5 177 0
8 * mu. Peg PM* 22 50 00.1930748087 +24 36 05.692620534 5.10 4.42 3.48 2.80 2.33 G8+III 304 0

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