1998BaltA...7..299M

Query : 1998BaltA...7..299M

1998BaltA...7..299M - Baltic Astronomy, 7, 299-311 (1998/April-0)

Should roAp stars get WET and will they make a splash?

MATTHEWS J.

Abstract (from CDS):

The one attempt (in 1989) to monitor a rapidly oscillating Ap (roAp) star with the WET network was a failure, but for reasons which are now clearly recognized and correctable. In the meantime, roAp research has blossomed to the point that we are better able to extract astrophysical information about these magnetic stars from WET-quality data. The time is ripe for a WET campaign on a multi-mode roAp pulsator.

Abstract Copyright: ∼

Journal keyword(s): stars: chemically peculiar, magnetic, oscillations, asteroseismology

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 V* DO Eri a2* 03 55 16.1313315312 -12 05 56.727712752 6.35 6.32 6.00     A9VpSrEuCr 411 0
2 HD 83368 a2* 09 36 25.4255061727 -48 45 04.240404102   6.49 6.23     A8VSrCrEu 277 0
3 V* V816 Cen dS* 11 37 37.0409608152 -46 42 34.877876832 8.99 8.79 8.03     F8/G0p 332 0
4 * alf Cir a2* 14 42 30.4206520931 -64 58 30.478845491 3.55 3.43 3.19 2.96 2.86 A7VpSrCrEu 384 0
5 * 33 Lib a2* 15 29 34.7424021408 -17 26 27.377921220 7.22 7.07 6.69     F0VspEuGdSr 260 0
6 V* V694 CrA a2* 18 12 25.8347418984 -37 45 09.271268532   8.34 7.92     ApSrCrEu 122 0

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