Measuring differential rotation of the K-giant $ Andromedae

Z. KH ovári, H. Korhonen, L. Kriskovics, K. Vida, J.-F. Donati, H. Le Coroller, J.~D. Monnier, E. Pedretti, P. Petit

Research output: Contribution to journalArticle

Abstract

Aims. We investigate the temporal spot evolution of the K-giant component in the RS CVn-type binary system ζ Andromedae to establish its surface differential rotation.

Methods. Doppler imaging was used to study three slightly overlapping spectroscopic datasets, which were obtained independently at three different observing sites. Each dataset covers one full stellar rotation with good phase coverage, which results in a continuous coverage of almost three stellar rotations (Prot = 17.8 d). Therefore, these data are well-suited for reconstructing surface temperature maps and studying temporal evolution in spot configurations. Surface differential rotation was measured by the means of cross-correlation of all possible image pairs.

Results. The individual Doppler reconstructions agree well in the revealed spot pattern, recovering numerous low-latitude spots with temperature contrasts of up to ≈1000 K with respect to the unspotted photosphere, and also an asymmetric polar cap that is diminishing with time. Our detailed cross-correlation study consistently indicates solar-type differential rotation with an average surface shear α ≈ 0.055, in agreement with former results.
Original languageEnglish
Pages (from-to)A50
JournalAstronomy and Astrophysics
Volume539
Early online date23 Feb 2012
DOIs
Publication statusPublished - 1 Mar 2012

Fingerprint

stellar rotation
cross correlation
polar caps
photosphere
tropical regions
surface temperature
shear
configurations
temperature

Keywords

  • stars: activity, stars: imaging, stars: late-type, starspots, stars: individual: $Andromedae

Cite this

KH ovári, Z., Korhonen, H., Kriskovics, L., Vida, K., Donati, J-F., Le Coroller, H., ... Petit, P. (2012). Measuring differential rotation of the K-giant $ Andromedae. Astronomy and Astrophysics, 539, A50. https://doi.org/10.1051/0004-6361/201118177
KH ovári, Z. ; Korhonen, H. ; Kriskovics, L. ; Vida, K. ; Donati, J.-F. ; Le Coroller, H. ; Monnier, J.~D. ; Pedretti, E. ; Petit, P. / Measuring differential rotation of the K-giant $ Andromedae. In: Astronomy and Astrophysics. 2012 ; Vol. 539. pp. A50.
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KH ovári, Z, Korhonen, H, Kriskovics, L, Vida, K, Donati, J-F, Le Coroller, H, Monnier, JD, Pedretti, E & Petit, P 2012, 'Measuring differential rotation of the K-giant $ Andromedae', Astronomy and Astrophysics, vol. 539, pp. A50. https://doi.org/10.1051/0004-6361/201118177

Measuring differential rotation of the K-giant $ Andromedae. / KH ovári, Z.; Korhonen, H.; Kriskovics, L.; Vida, K.; Donati, J.-F.; Le Coroller, H.; Monnier, J.~D.; Pedretti, E.; Petit, P.

In: Astronomy and Astrophysics, Vol. 539, 01.03.2012, p. A50.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Measuring differential rotation of the K-giant $ Andromedae

AU - KH ovári, Z.

AU - Korhonen, H.

AU - Kriskovics, L.

AU - Vida, K.

AU - Donati, J.-F.

AU - Le Coroller, H.

AU - Monnier, J.~D.

AU - Pedretti, E.

AU - Petit, P.

PY - 2012/3/1

Y1 - 2012/3/1

N2 - Aims. We investigate the temporal spot evolution of the K-giant component in the RS CVn-type binary system ζ Andromedae to establish its surface differential rotation.Methods. Doppler imaging was used to study three slightly overlapping spectroscopic datasets, which were obtained independently at three different observing sites. Each dataset covers one full stellar rotation with good phase coverage, which results in a continuous coverage of almost three stellar rotations (Prot = 17.8 d). Therefore, these data are well-suited for reconstructing surface temperature maps and studying temporal evolution in spot configurations. Surface differential rotation was measured by the means of cross-correlation of all possible image pairs.Results. The individual Doppler reconstructions agree well in the revealed spot pattern, recovering numerous low-latitude spots with temperature contrasts of up to ≈1000 K with respect to the unspotted photosphere, and also an asymmetric polar cap that is diminishing with time. Our detailed cross-correlation study consistently indicates solar-type differential rotation with an average surface shear α ≈ 0.055, in agreement with former results.

AB - Aims. We investigate the temporal spot evolution of the K-giant component in the RS CVn-type binary system ζ Andromedae to establish its surface differential rotation.Methods. Doppler imaging was used to study three slightly overlapping spectroscopic datasets, which were obtained independently at three different observing sites. Each dataset covers one full stellar rotation with good phase coverage, which results in a continuous coverage of almost three stellar rotations (Prot = 17.8 d). Therefore, these data are well-suited for reconstructing surface temperature maps and studying temporal evolution in spot configurations. Surface differential rotation was measured by the means of cross-correlation of all possible image pairs.Results. The individual Doppler reconstructions agree well in the revealed spot pattern, recovering numerous low-latitude spots with temperature contrasts of up to ≈1000 K with respect to the unspotted photosphere, and also an asymmetric polar cap that is diminishing with time. Our detailed cross-correlation study consistently indicates solar-type differential rotation with an average surface shear α ≈ 0.055, in agreement with former results.

KW - stars: activity, stars: imaging, stars: late-type, starspots, stars: individual: $Andromedae

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JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

SN - 0004-6361

ER -

KH ovári Z, Korhonen H, Kriskovics L, Vida K, Donati J-F, Le Coroller H et al. Measuring differential rotation of the K-giant $ Andromedae. Astronomy and Astrophysics. 2012 Mar 1;539:A50. https://doi.org/10.1051/0004-6361/201118177