2006BaltA..15..219S


Query : 2006BaltA..15..219S

2006BaltA..15..219S - Baltic Astronomy, 15, 219-226 (2006/April-0)

Line-profile variations in pulsating sdB stars as a pulsation mode diagnostic.

SCHOENAERS C. and LYNAS-GRAY A.E.

Abstract (from CDS):

In previous attempts to perform seismic modeling of pulsating subdwarf-B stars, various mode identification techniques are used with uncertain results. We investigated a method so far neglected in sdB stars, but very successful for main-sequence pulsators, i.e., mode identification from the line-profile variations caused by stellar pulsation. We report the calculation of time-resolved synthetic spectra for sdB stars pulsating with various combinations of pulsation modes; these calculations were carried out over appropriate ranges of effective temperature, surface gravity and helium abundances. Preliminary tests using these synthetic line-profile variations demonstrated their potential for mode identification by comparison with observations.

Abstract Copyright:

Journal keyword(s): stars: hot subdwarfs - stars: oscillations

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 PG 0014+068 HS* 00 16 54.2537878176 +07 04 30.043437816   15.3       sdO 73 1
2 V* EO Cet HS* 01 23 43.2471248112 -05 05 45.831024564   12.21 12.65     sdOV+F4V 65 0
3 HD 74194 HXB 08 40 47.7915253032 -45 03 30.235569624 7.05 7.77 7.55 8.70   O8.5Ib-II(f)p 209 0
4 PG 1219+534 HS* 12 21 29.0914917288 +53 04 36.796062144   12.41       sdB 84 1
5 PG 1325+102 HS* 13 27 48.5600155368 +09 54 51.049107756   13.73 13.98 14.29   sdBO 57 1
6 ESO 136-6 Sy2 15 53 35.3846505552 -61 40 59.036145456           ~ 43 0
7 PG 1605+072 HS* 16 08 03.6872637792 +07 04 28.748468964   12.53 12.83 13.18   sdB0.2VIHe3 133 0
8 KPD 1930+2752 HS* 19 32 14.8088063952 +27 58 35.445679608 12.80 13.75 13.82     sdB 159 0
9 KPD 2109+4401 HS* 21 11 47.6445824136 +44 13 50.620755936 12.14 13.11 13.30 13.64   sdB 67 0
10 PHL 44 HS* 21 35 13.3327203264 -13 33 22.555121148 11.77 12.86 13.16     sdB 21 0

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