1998A&A...337..790A


Query : 1998A&A...337..790A

1998A&A...337..790A - Astronomy and Astrophysics, volume 337, 790-796 (1998/9-3)

The discovery of new γ Doradus stars from the HIPPARCOS mission.

AERTS C., EYER L. and KESTENS E.

Abstract (from CDS):

We present a classification of 39 new variable stars with spectral type between A2 and F8 discovered by Hipparcos with the aim to find new γ Doradus stars. We have used a multivariate classification scheme and report the discovery of 14 new γ Doradus variables among this unbiased sample. Our results point out the biased nature towards hot temperatures of earlier, ground-based surveys of these variables. The coolest star among our sample has an effective temperature only slightly hotter than 6000K. For most of the 14 new γ Doradus stars, we are able to detect more than one period in the Hipparcos light curve. The multiperiodicity points towards the presence of high-order g-modes. In view of the lack of a pulsation mechanism for these objects, we determine their position in the HR diagram with respect to the δ Scuti stars.

Abstract Copyright:

Journal keyword(s): stars: variables: other - stars: oscillations - stars: statistics - methods: statistical

Simbad objects: 22

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Number of rows : 22
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 * alf Tri SB* 01 53 04.9054187154 +29 34 43.747211027 3.96 3.90 3.42 3.00 2.72 F5III 288 0
2 V* FG Eri EB* 01 55 48.2503151016 -55 04 19.821740952   6.87 6.71     A5V 32 0
3 V* EP Cet gD* 02 24 09.5673209112 -16 15 15.483977928   6.96 6.67     F0IV/V 51 0
4 * 50 Per RS* 04 08 36.6171573432 +38 02 23.058806100 7.78 5.97   5.2   F8V 218 0
5 * gam Dor gD* 04 16 01.5866224848 -51 29 11.932714356   4.55 4.20     F1V 314 0
6 V* AC Lep gD* 06 00 17.6604502536 -12 54 00.121230396   6.548 6.195     F2IV 52 0
7 HD 58634 * 07 24 47.0033480232 -37 17 22.871401368   7.11 6.87 6.95   A9IIIb 21 0
8 V* UY UMi gD* 12 15 20.2712485488 +87 42 00.426459852   6.590 6.259     F1IV 58 0
9 V* V1026 Cen gD* 12 51 50.7460909104 -52 07 43.288390128   9.60 9.23     A(3)mA5-A7 20 0
10 * 8 Dra gD* 12 55 28.5485641728 +65 26 18.507128532   5.516 5.225     F3IV 94 0
11 V* V947 Cen dS* 13 05 06.6587749992 -47 07 00.868435860   6.843 6.426     F3III 39 0
12 V* OP Aps dS* 15 24 32.4722996784 -80 26 26.256479964   8.46 8.08     A9III 17 0
13 * iot TrA SB* 16 27 57.3455455848 -64 03 28.585517400   5.61 5.29     F0IV 61 1
14 V* V872 Ara gD* 16 40 44.3994563352 -51 28 41.726953560   6.58 6.29     F1Vnnm-4 42 0
15 V* V2118 Oph gD* 18 01 33.2032926288 +11 17 08.732552604   7.37 7.01     F2IV-V 70 0
16 V* V2502 Oph gD* 18 17 04.8404548584 +01 00 20.632225968   6.91 6.61     F2V 109 0
17 V* V349 Tel gD* 19 50 08.3604248064 -50 36 09.145076940   7.89 7.60     F2V 25 0
18 V* BD Cap dS* 20 10 06.7541961552 -25 17 02.442930756   7.87 7.44     A9III 31 0
19 HD 214291 SB* 22 37 47.7333864360 -39 51 25.611689988   7.12 6.59     F7V 29 0
20 V* EE Tuc gD* 22 57 59.4338327640 -59 05 22.198067700   7.03 6.69     F2V 32 0
21 V* DI Gru EB* 23 06 48.0111314304 -38 47 38.801021604   9.07 8.70     F3IV 22 0
22 HD 218396 El* 23 07 28.7157209544 +21 08 03.310767492   6.21 5.953     F0+VkA5mA5 1141 0

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