2000A&AS..145..275N

Query : 2000A&AS..145..275N

2000A&AS..145..275N - Astron. Astrophys., Suppl. Ser., 145, 275-281 (2000/August-0)

A three-year Stroemgren photometric survey of suspected β Pictoris-like stars.

NITSCHELM C., LECAVELIER DES ETANGS A., VIDAL-MADJAR A., FERLET R., OLSEN E.H. and DENNEFELD M.

Abstract (from CDS):

We carried out a Stroemgren photometric survey of thirteen southern bright stars, including β Pictoris itself, during three years, d'Astrophysique de Paris, in order to detect possible weak photometric variations. β Pictoris presents a small long-term variation with a change of brightness by -2.1x10–3 mag per year, over about two years from beginning of 1996, a situation relatively similar to the one about 18 years ago. Among the other stars, only HD 38392 presents weak photometric variations with a period of 21.4 days, probably related to the star rotation period. The negative result concerning photometric variations of all other stars suggests that those stars are actually really stable and strengthens the reality of the variations discovered in the case of β Pictoris and HD 38392.

Abstract Copyright: ∼

Journal keyword(s): stars: beta Pic - circumstellar matter - planetary systems - Stroemgren photometry

VizieR on-line data: <Available at CDS (J/A+AS/145/275): stars.dat tables.dat>

Simbad objects: 35

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Number of rows : 35
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 HD 203 PM* 00 06 50.0863238088 -23 06 27.145662264   6.547 6.173   5.74 F3V 129 0
2 HD 256 ** 00 07 18.2658367200 -17 23 13.173158760   6.311 6.203 7.36   A3Vn_sh 108 0
3 * 6 Cet PM* 00 11 15.8580395472 -15 28 04.720468404 5.35 5.38 4.89     F8VFe-0.8CH-0.5 312 0
4 * lam02 For PM* 02 36 58.6077493776 -34 34 40.711246464 6.67 6.45 5.79     G1V 213 1
5 * gam02 For PM* 02 49 54.1826368200 -27 56 31.139469636   5.384 5.377     A1V 40 0
6 * alf For PM* 03 12 04.5298039833 -28 59 15.439152331 4.41 4.51 3.98 3.39 3.08 F6V 272 0
7 * v Eri * 03 30 37.0583178770 -05 04 30.532729396   4.631 4.725     B9III 85 0
8 * eps Eri BY* 03 32 55.8444911587 -09 27 29.739493865 5.19 4.61 3.73 3.00 2.54 K2V 1932 1
9 HD 22243 * 03 34 37.4713793840 -09 52 05.732668974   6.258 6.239     A0V 35 0
10 * 21 Eri PM* 03 39 01.1165151744 -05 37 34.368381948   6.88 5.96     K0IV 62 0
11 HD 25069 RG* 03 58 52.3939149216 -05 28 11.811149040   6.848 5.833     K0/1III 74 0
12 HD 26676 * 04 13 34.5706402104 +10 12 44.918270316   6.268 6.249     B8V 100 1
13 HD 26703 * 04 13 49.8380933616 +12 45 13.345753356   7.40 6.25     K0 26 0
14 HD 26793 * 04 14 36.2326070880 +10 00 41.065922196   5.118 5.218     B9Vn 62 0
15 * omi02 Eri Er* 04 15 16.3196189945 -07 39 10.330779018 5.69 5.25 4.43 3.74 3.29 K0V 814 0
16 * eta01 Pic PM* 05 02 48.6860731776 -49 09 05.062859424   5.796 5.372     F5V 70 0
17 * zet Dor PM* 05 05 30.6556741368 -57 28 21.736898832   5.215 4.708     F9VFe-0.5 238 0
18 * zet Pic PM* 05 19 22.1350114344 -50 36 21.481796808   5.96 5.45     F6IV 88 0
19 * kap Pic * 05 22 22.1468864184 -56 08 03.836012676   5.997 6.086     B8/9V 49 0
20 HD 35386 * 05 23 11.9929615632 -26 42 19.553959512   6.970 6.490     F6V 47 0
21 * 29 Dor Be* 05 36 54.9785586360 -66 33 37.027712484   6.221 6.274     A1IIIe 55 0
22 V* AK Lep BY* 05 44 26.5367235521 -22 25 18.614500501   7.09 6.15     K3 165 0
23 * gam Lep PM* 05 44 27.7906169580 -22 26 54.187756254 4.08 4.07 3.60 3.15 2.89 F6V 428 0
24 HD 38382 * 05 44 28.3954021848 -20 07 35.661845280   6.898 6.341     F8.5V 96 0
25 * del Dor * 05 44 46.3699967519 -65 44 07.793159129 4.69 4.57 4.36 4.10 3.93 A7V 128 0
26 * zet Lep * 05 46 57.3413646658 -14 49 19.020570470   3.637 3.525     A2IV-V(n) 296 0
27 * bet Pic PM* 05 47 17.0876901 -51 03 59.441135 4.13 4.03 3.86 3.74 3.58 A6V 1902 1
28 HD 39963 * 05 51 23.0854945344 -64 02 00.827621952   7.215 6.359     G8III 22 0
29 HD 40200 * 05 54 41.1200582952 -49 37 37.237826280   5.940 6.098     B3III 38 0
30 HD 41692 * 06 06 38.7363839832 -04 11 37.808375208 4.71 5.231 5.362     B5II/III 128 0
31 HD 42111 * 06 08 57.9037271424 +02 29 58.885200456 5.86 5.80 5.73     B9V 125 0
32 HD 42824 * 06 12 44.5945739856 -02 30 17.335091196   6.666 6.616     A1V 44 0
33 HD 155450 bC? 17 12 58.5578949696 -32 26 17.993977116 5.36 6.019 5.997 7.21   B1Ib 64 0
34 * c Oph Be* 17 31 24.9538710166 -23 57 45.514802684 4.75 4.81 4.81 4.74 4.72 A0V 273 0
35 * 58 Oph PM* 17 43 25.7935382141 -21 40 59.498912759   5.313 4.861     F5V 146 0

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