2000MNRAS.314..162B


Query : 2000MNRAS.314..162B

2000MNRAS.314..162B - Mon. Not. R. Astron. Soc., 314, 162-174 (2000/May-1)

Doppler images from dual-site observations of southern rapidly rotating stars - I. Differential rotation on PZ Tel.

BARNES J.R., COLLIER CAMERON A., JAMES D.J. and DONATI J.-F.

Abstract (from CDS):

We present Doppler images of the young, late-type star PZ Tel from spectroscopic observations at two epochs. The 0.95-d period necessitated dual-site observations in order to obtain full phase coverage. The resulting maximum entropy reconstructions based on least-squares deconvolved profiles derived from ∼2800 photospheric absorption lines reveal the presence of starspots at all latitudes. By cross-correlation of constant-latitude strips from the images, we derive a measure of rotation as a function of latitude. The rate of surface shear is found to be in close agreement with the solar value. Hα absorption transients reveal several prominences to be present at the time of observation. We also examine further evidence for the young evolutionary status of PZ Tel through radial velocity, and lithium abundance.

Abstract Copyright: 2000, Royal Astronomical Society

Journal keyword(s): line: profiles - methods: data analysis - stars: activity - stars: individual: PZ Tel - stars: late-type - stars: rotation

Simbad objects: 28

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Number of rows : 28
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 * 6 Cet PM* 00 11 15.8580395472 -15 28 04.720468404 5.35 5.38 4.89     F8VFe-0.8CH-0.5 334 0
2 * alf Eri Be* 01 37 42.84548 -57 14 12.3101 -0.36 0.30 0.46 0.49 0.60 B6Vpe 495 1
3 NGC 1039 OpC 02 42 09.1 +42 44 02           ~ 467 0
4 HD 19007 * 03 02 01.7540866440 -41 50 12.487366140   9.764 9.221     K0III 19 0
5 V* V484 Per BY* 03 22 21.9201012551 +49 08 27.732216837   12.07 11.37     G6V 78 0
6 V* V532 Per BY* 03 26 22.2275044296 +49 25 37.501937904   11.98 11.27     G2-3V 76 0
7 Cl Melotte 20 MGr 03 26 50.6 +48 51 48           ~ 928 0
8 Cl Melotte 22 OpC 03 46 38.0 +24 10 41           ~ 3679 0
9 V* V471 Tau SB* 03 50 24.9666549840 +17 14 47.430910716   10.258 9.373   8.393 K2V+DA 697 0
10 HD 36187 PM* 05 28 15.3350066568 -37 13 50.747659536   5.575 5.552   5.52 A0V 40 0
11 V* AB Dor TT* 05 28 44.8712165880 -65 26 55.199147208 8.259 7.856 6.999 6.496 5.993 K0V 1080 0
12 NGC 2516 OpC 07 58 00.5 -60 46 36           ~ 793 0
13 V* LQ Hya BY* 09 32 25.5683895648 -11 11 04.692242760 9.316 8.761 7.891 7.288 6.815 K1Vp 480 0
14 IC 2602 OpC 10 42 55.9 -64 25 22           ~ 735 0
15 * pi. Cen ** 11 21 00.4170807171 -54 29 27.964002014           B5Vn 127 0
16 CD-31 9113 PM* 11 35 26.9477670462 -32 32 23.884215079 12.508 11.322 9.813 8.821 7.664 M2V 188 1
17 HD 109200 PM* 12 33 31.3825438408 -68 45 20.912700882 8.472 7.987 7.140 6.661 6.237 K1V 142 0
18 HD 118972 PM* 13 41 04.1705560968 -34 27 50.962695660 8.278 7.78 6.92 6.448 8.390 K0V 114 0
19 HD 119850 PM* 13 45 43.7755597223 +14 53 29.471707437 10.989 9.894 8.50 7.465 6.363 M2V 402 0
20 HD 125072 PM* 14 19 04.8342927813 -59 22 44.536555365   7.69 6.66     K3IV 169 0
21 V* EK Dra BY* 14 39 00.2104038120 +64 17 29.979649860   8.243 7.604     G5VFe-0.7CH-1(k) 500 0
22 * ksi Boo BY* 14 51 23.37993 +19 06 01.6994 5.618 5.370 4.593 3.91 3.48 G7Ve+K5Ve 503 0
23 HD 145417 PM* 16 13 48.5588453721 -57 34 13.843989664 8.663 8.365 7.540 7.054 6.588 K3VFe-1.7 173 0
24 HD 157881 PM* 17 25 45.2324302566 +02 06 41.123732402 10.126 8.865 7.56 6.649 5.89 K7V 361 0
25 V* PZ Tel BY* 18 53 05.8735056984 -50 10 49.897437168   9.22 8.342   7.464 G9IV 364 0
26 * sig Sgr ** 18 55 15.92650 -26 17 48.2068 1.06 1.923 2.067     B2.5V 284 1
27 HD 202917 PM* 21 20 49.9576157736 -53 02 03.155667216   9.32 8.67   7.882 G7V 191 0
28 HD 224618 PM* 23 59 27.8819655183 -16 56 40.929610806   9.69 8.96     K0V 76 0

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