2012MNRAS.421..132G


Query : 2012MNRAS.421..132G

2012MNRAS.421..132G - Mon. Not. R. Astron. Soc., 421, 132-148 (2012/March-3)

FR Cnc revisited: photometry, polarimetry and spectroscopy.

GOLOVIN A., GALVEZ-ORTIZ M.C., HERNAN-OBISPO M., ANDREEV M., BARNES J.R., MONTES D., PAVLENKO E., PANDEY J.C., MARTINEZ-ARNAIZ R., MEDHI B.J., PARIHAR P.S., HENDEN A., SERGEEV A., ZAITSEV S.V. and KARPOV N.

Abstract (from CDS):

This paper is part of a multiwavelength study aimed at using complementary photometric, polarimetric and spectroscopic data to achieve an understanding of the activity process in late-type stars. Here, we present the study of FR Cnc, a young, active and spotted star.

We performed analysis of All Sky Automated Survey 3 (ASAS-3) data for the years 2002-08 and amended the value of the rotational period to be 0.826518 d. The amplitude of photometric variations decreased abruptly in the year 2005, while the mean brightness remained the same, which was interpreted as a quick redistribution of spots. BVRC and ICbroad-band photometric calibration was performed for 166 stars in FR Cnc vicinity.

The photometry at Terskol Observatory shows two brightening episodes, one of which occurred at the same phase as the flare of 2006 November 23. Polarimetric BVR observations indicate the probable presence of a supplementary source of polarization. We monitored FR Cnc spectroscopically during the years 2004-08. We concluded that the radial velocity changes cannot be explained by the binary nature of FR Cnc. We determined the spectral type of FR Cnc as K7V. Calculated galactic space-velocity components (U, V, W) indicate that FR Cnc belongs to the young disc population and might also belong to the IC 2391 moving group. Based on Li Iλ6707.8 measurement, we estimated the age of FR Cnc to be between 10 and 120 Myr. Doppler tomography was applied to create a starspot image of FR Cnc. We optimized the goodness of fit to the deconvolved profiles for axial inclination, equivalent width and v sin i, finding v sin i=46.2 km/s and i= 55°. We also generated a synthetic V-band light curve based on Doppler imaging that makes simultaneous use of spectroscopic and photometric data. This synthetic light curve displays the same morphology and amplitude as the observed one.

The starspot distribution of FR Cnc is also of interest since it is one of the latest spectral types to have been imaged. No polar spot was detected on FR Cnc.


Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): stars: activity - stars: flare - stars: individual: FR Cnc - stars: rotation

Simbad objects: 15

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Number of rows : 15
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 V* VY Ari RS* 02 48 43.7287198695 +31 06 54.592461256   7.72   6.4   G9 241 0
2 V* CC Cas SB* 03 14 05.3361655368 +59 33 48.485582712 7.07 7.56 7.08     O8.5III(n)((f)) 308 0
3 HD 21447 * 03 30 00.1828170168 +55 27 06.506069256 5.160 5.140 5.090 5.01 5.02 A1Va 147 0
4 HD 25433 * 04 02 16.3535768280 -04 18 09.865994220   9.81 8.70     K1III 15 0
5 BD+52 913 WD* 05 05 30.6180977592 +52 49 51.919301604 10.25 11.44 11.69 11.93 12.108 DA.8 1153 0
6 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
7 V* FR Cnc BY* 08 32 30.5296878048 +15 49 26.229486900   11.42 10.25 9.788   K7e 41 0
8 IC 2391 OpC 08 41 17.5 -53 03 00           ~ 871 0
9 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
10 V* MS Ser BY* 15 58 43.9452509832 +25 34 10.427623284   9.21 8.347   7.201 G/K:e 110 0
11 HD 151877 PM* 16 48 35.5141646014 +37 00 48.123002986   9.22   7.9   K0V 100 0
12 V* EY Dra BY* 18 16 16.7795336184 +54 10 21.732232332   13.69 11.84     dM1.5e 75 0
13 BD+22 4409 BY* 21 31 01.7140062576 +23 20 07.374015564   10.240 9.245 8.6 7.965 K3Vke 187 0
14 V* HK Aqr BY* 23 08 19.5510173448 -15 24 35.766079704 13.4 12.282 10.872 9.964 9.019 M0Ve 219 0
15 NAME IC 2391 Moving Group MGr ~ ~           ~ 27 0

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