2004BaltA..13..573K


Query : 2004BaltA..13..573K

2004BaltA..13..573K - Baltic Astronomy, 13, 573-580 (2004/October-0)

Carbon stars in the UVES Paranal Observatory project.

KIPPER T.

Abstract (from CDS):

The high resolution spectra of five cool carbon stars (X TrA, TW Hor, W Ori, U Ant and U Hya) obtained in the UVES Paranal Observatory Project were used to examine the quality of R. A. Bell's line-list for synthesizing the spectra of cool carbon stars. We propose the improvements of this line-list and estimate the abundances of several chemical elements.

Abstract Copyright: ∼

Journal keyword(s): stars: atmospheres - stars: carbon - stars: individual (X TrA, TW Hor, W Ori, U Ant, U Hya)

Simbad objects: 6

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Number of rows : 6
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 NGC 1252 err 03 10 49 -57 46.0           ~ 38 0
2 V* TW Hor C* 03 12 33.1599109680 -57 19 17.577229512   7.93 5.71 3.78 2.40 C-N5IIIb: 143 0
3 V* W Ori C* 05 05 23.7190712856 +01 10 39.454639032 16.36 9.52 6.10 3.83 2.35 C-N5 300 0
4 V* U Ant C* 10 35 12.8510147472 -39 33 45.324020448 15.32 8.22 5.38 3.18 1.86 C-N3 162 0
5 V* U Hya C* 10 37 33.2729535 -13 23 04.352923 13.29 7.51 4.82 3.05 1.78 C-N5 314 0
6 V* X TrA C* 15 14 19.1755012584 -70 04 46.113298104 15.88 9.19 5.81     C5,5 130 0

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