2008A&A...489..911E


Query : 2008A&A...489..911E

2008A&A...489..911E - Astronomy and Astrophysics, volume 489911-921 (2008/10-2)

Polarimetric measures of selected variable stars.

ELIAS II N.M., KOCH R.H. and PFEIFFER R.J.

Abstract (from CDS):

The purpose of this paper is to summarize and interpret unpublished optical polarimetry for numerous program stars that were observed over the past decades at the Flower and Cook Observatory (FCO), University of Pennsylvania. We also make the individual calibrated measures available for long-term comparisons with new data. We employ three techniques to search for intrinsic variability within each dataset. First, when the observations for a given star and filter are numerous enough and when a period has been determined previously via photometry or spectroscopy, the polarimetric measures are plotted versus phase. If a statistically significant pattern appears, we attribute it to intrinsic variability. Second, we compare means of the FCO data to means from other workers. If they are statistically different, we conclude that the object exhibits long-term intrinsic variability. Third, we calculate the standard deviation for each program star and filter and compare it to the standard deviation estimated from comparable polarimetric standards. If the standard deviation of the program star is at least three times the value estimated from the polarimetric standards, the former is considered intrinsically variable. All of these statements are strengthened when variability appears in multiple filters. We confirm the existence of an electron-scattering cloud at L1 in the β Per system, and find that LY Aur and HR 8281 possess scattering envelopes. Intrinsic polarization was detected for Nova Cas 1993 as early as day +3. We detected polarization variability near the primary eclipse of 32 Cyg. There is marginal evidence for polarization variability of the β Cepheid type star γ Peg. The other objects of this class exhibited no variability. All but one of the β Cepheid objects (ES Vul) fall on a tight linear relationship between linear polarization and E(B-V), in spite of the fact that the stars lay along different lines of sight. This dependence falls slightly below the classical upper limit of Serkowski, Mathewson, and Ford.

Abstract Copyright: ∼

Journal keyword(s): polarization - binaries: close - Cepheids - circumstellar matter - accretion, accretion disks - dust, extinction

VizieR on-line data: <Available at CDS (J/A+A/489/911): stars.dat table12.dat table.dat>

Simbad objects: 47

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Number of rows : 47
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 * 33 Psc RS* 00 05 20.1411719640 -05 42 27.431698821 6.52 5.65 4.61 3.83 3.29 K0III-IV 223 0
2 * 5 Cet SB* 00 08 12.0955513656 -02 26 51.740585628   7.58 6.22     K2IIICNIVp 127 0
3 HD 232121 SB* 00 10 42.0679172568 +54 53 29.361482988   9.67 8.97     B5+K3III 186 0
4 * gam Peg bC* 00 13 14.1523490172 +15 11 00.954346538 1.75 2.61 2.84 2.94 3.13 B2IV 720 0
5 * zet And El* 00 47 20.3257188471 +24 16 01.842781713 6.05 5.18 4.06 3.21 2.62 K1III+KV 299 0
6 * 53 Ari bC* 03 07 25.6731510240 +17 52 47.969633820 5.18 5.997 6.117     B1.5V 146 1
7 * bet Per SB* 03 08 10.1324535 +40 57 20.328013 1.70 2.07 2.12 2.08 2.11 B8V 1265 1
8 HD 25638 EB* 04 07 49.2849421032 +62 19 58.626896088 6.82 7.26 6.93     O9.5Vn 227 1
9 NGC 1502 OpC 04 07 49.4 +62 19 35   7.47 6.9     ~ 202 1
10 HD 30353 sg* 04 48 53.3476200024 +43 16 32.086716960 8.05 8.22 7.76     A5Iap 149 0
11 * eps Aur SB* 05 01 58.1343686760 +43 49 23.917115316 3.86 3.53 2.99 2.47 2.02 A9Ia 600 0
12 * alf Aur SB* 05 16 41.35871 +45 59 52.7693 1.33 0.88 0.08 -0.52 -0.96 G3III: 1207 0
13 * 17 Aur SB* 05 18 18.8960529504 +33 46 02.516925540   6.102 6.144     B9V+B9.5V 308 0
14 * eta Ori bC* 05 24 28.61672 -02 23 49.7311 2.25 3.18 3.35 3.44 3.65 B1V+B2: 412 0
15 HD 35921 ** 05 29 42.6497086888 +35 22 30.097742031 6.23         O9II 255 0
16 * del Ori ** 05 32 00.40009 -00 17 56.7424 0.96 2.02 2.41 2.32 2.54 O9.5IINwk 796 0
17 * del02 Ori SB* 05 32 00.4064140728 -00 17 04.347484800 5.97 6.67 6.83     B2Vsn 296 0
18 HD 43246 SB* 06 16 22.1977904160 +28 51 07.127565372   7.82 7.41     A0Vn+F5III 51 0
19 V* UX Mon SB* 07 59 16.3752271920 -07 30 17.892250632   8.74 8.42     A2/3+G/K 133 0
20 * 23 Sex Pu* 10 21 02.0059724664 +02 17 22.997775480 5.9 6.547 6.644     B2IV/V 114 0
21 V* TX UMa SB* 10 45 20.5041244512 +45 33 58.708181052   6.99 6.98     B8V+G0III-IV 291 0
22 * alf Vir bC* 13 25 11.57937 -11 09 40.7501 -0.20 0.74 0.97 1.06 1.30 B1V 877 1
23 * del Lib SB* 15 00 58.3483018872 -08 31 08.210408772 4.82 4.93 4.93 4.85 4.84 A0V 305 0
24 * alf CrB SB* 15 34 41.2684881676 +26 42 52.866000089 2.19 2.22 2.24 2.21 2.25 A1IV 499 0
25 V* V600 Her SB* 16 36 58.2040305408 +14 28 30.910523016 5.87 6.845 7.028     B0.5III 165 0
26 * bet Lyr SB* 18 50 04.7951442356 +33 21 45.600371200 2.85 3.42 3.42 3.31 3.29 B8.5Ib-II 955 0
27 * 2 Vul Pu* 19 17 43.6353905520 +23 01 31.941802308 4.64 5.43 5.43     B1IIIn 146 0
28 V* V1143 Cyg SB* 19 38 41.1829269072 +54 58 25.647010572       5.6   F6Va 229 0
29 V* V380 Cyg SB* 19 50 37.3267754400 +40 35 59.135141652 4.86 5.613 5.680     B1.1III+B2.5/3V: 305 0
30 * 31 Cyg SB* 20 13 37.9082370480 +46 44 28.761618048 5.50 5.08 3.80 2.83 2.07 K3Ib+B2IV-V 385 0
31 * omi02 Cyg SB* 20 15 28.3242122880 +47 42 51.213932496 6.54 5.50 3.98 2.78 1.86 K7Ib-II+B1V 347 0
32 HD 198288 SB* 20 47 59.5845423048 +39 17 15.717392988 8.080 7.72 7.06     A3Ibep 213 0
33 V* Y Cyg SB* 20 52 03.5771840640 +34 39 27.486121104 6.31 7.23 7.32     O9.5IV+O9.5IV 382 0
34 V* BW Vul bC* 20 54 22.3947588600 +28 31 19.190976132 5.47 6.40 6.54     B2IIIv 301 0
35 HD 206267 Y*O 21 38 57.6195772032 +57 29 20.554016280 5.09 5.83 5.62   5.56 O6.0V((f))+O9:V 520 0
36 * del Cap SB* 21 47 02.4442395 -16 07 38.233507 3.22 3.12 2.83 2.59 2.43 kA5hF0mF2III 284 0
37 * 14 Cep SB* 22 02 04.5726270264 +58 00 01.309758516 4.77 5.551 5.542     O9IV(n)var+B1:V: 262 0
38 * 12 Lac bC* 22 41 28.6495065456 +40 13 31.609736580 4.24 5.080 5.229     B1.5III 369 0
39 V* AH Cep SB* 22 47 52.9412851944 +65 03 43.795145556 6.53 7.10 6.88     B0.2V+B2V 227 0
40 * 16 Lac bC* 22 56 23.6299283136 +41 36 13.948480440 4.61 5.436 5.587     B2IVs 325 0
41 HD 217811 V* 23 02 45.1478611209 +44 03 31.498436363 5.8 6.38 6.42     B2V 85 1
42 HD 218066 Be* 23 04 02.2270838832 +63 23 48.722060508 7.50 7.97 7.6     B1.5Vn 290 0
43 NAME III CEP ASSOC As* 23 04.2 +63 24           ~ 332 0
44 V* AR Cas SB* 23 30 01.9406369832 +58 32 56.112185112 4.18 4.760 4.886     B3V 222 0
45 V* V705 Cas No* 23 41 47.2354174125 +57 31 00.826200729       16.055   ~ 207 0
46 HD 224559 Be* 23 58 46.4393230728 +46 24 47.443832676 5.84 6.444 6.538     B4Vne 140 1
47 * ome Psc SB* 23 59 18.6902044464 +06 51 47.960421106       3.8   F4V 152 0

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