Magnetic activity of F stars

Slides:



Advertisements
Similar presentations
Stellar analysis system (SAS*) WP370 T. Appourchaux Institut d’Astrophysique Spatiale, Orsay *SAS= Special Air Service or Son Altesse Sérénissime.
Advertisements

1 The Sun as a whole: Rotation, Meridional circulation, and Convection Michael Thompson High Altitude Observatory, National Center for Atmospheric Research.
Solar-like Oscillations in Red Giant Stars Olga Moreira BAG.
The Independency of Stellar Mass-Loss Rates on Stellar X-ray Luminosity and Activity Space Telescope Science Institute – 2012.
Asteroseismology of solar-type stars Revolutionizing the study of solar-type stars Hans Kjeldsen, Aarhus University.
A ground-based velocity campaign on Procyon Tim Bedding (Univ. Sydney) and about 50 others.
Travis Metcalfe (SSI) Magnetic Activity Cycles and the Solar-Stellar Connection.
Southern HK project Metcalfe et al. (2009, arXiv: ) Small telescopes at CTIO run by SMARTS partners: Yale, GSU, STScI, et al. Service observing.
SEARCHING FOR PLANETS IN THE HABITABLE ZONE. FROM COROT TO PLATO Ennio Poretti – INAF OAB.
Prospects for asteroseismology of solar-like stars T. Appourchaux Institut d’Astrophysique Spatiale, Orsay.
Symposium CoRoT 2009 – Cité Universitaire – 2 February 2009 Analysis of power spectra of Sun-like stars using a Bayesian Approach Thierry Appourchaux Symposium.
Reaching the 1% accuracy level on stellar mass and radius determinations from asteroseismology Valerie Van Grootel (University of Liege) S. Charpinet (IRAP.
Exoplanet- Asteroseismology Synergies Bill Chaplin, School of Physics & Astronomy University of Birmingham, UK EAHS2012, Oxford, 2012 March 15.
Patrick Gaulme Thierry Appourchaux Othman Benomar Mode identification with CoRoT and Kepler solar- like oscillation spectra 1 SOHO-GONG XXIV, Aix en Provence.
Thanks to Henrietta Swan Leavitt, Harvard CfA November 5th Hommage to Henrietta Leavitt from the CoRoT Team Annie BAGLIN, Merième CHADID,
Catania 09/08SIAMOIS1/26 Benoît Mosser, for the SIAMOIS team Ground-based Doppler asteroseismology after CoRoT and Kepler.
Marc Pinsonneault (OSU).  New Era in Astronomy  Seismology  Large Surveys  We can now measure things which have been assumed in stellar modeling 
PLAnetary Transits and Oscillations of stars Thierry Appourchaux for the PLATO Consortium
Atomic Force Microscopy
Layers of the Solar Atmosphere Corona Chromosphere Photosphere Details of solar activity can be seen more easily in the hotter outer layers, which are.
1 CoRoT Highlights Annie Baglin and Eric Michel Observatoire de Paris and all the CoRoT Team and all the CoRoT Team * The Mission * Seismology * Stellar.
Katrien Uytterhoeven The Kepler space mission: New prospects for δ Sct, γ Dor, and hybrid stars Instituto de Astrofísica de Canarias, Tenerife NMSU, January.
Characterisation of stellar granulation and stellar activity (observational requirements, feasability, expectations) F. Baudin 1, R. Samadi 2, M-J Goupil.
Adriana V. R. Silva CRAAM/Mackenzie COROT /11/2005.
Astrostatistics, and Brown Dwarfs Chris Koen, Dept. Statistics, University of the Western Cape.
COROT Additional Programme Werner W. Weiss. 2 Seismology and Exoplanetary Field 0 E2 CCD A1CCD E1 CCD E2 CCD A2 XVXV YVYV Left Right 0 E1 3.05° 2.70°
Magnetic mapping of solar-type stars Pascal Petit figure: © M. Jardine.
MARTIN STILL – IAU XXVIII General Assembly – SpS #13: High-Precision Tests of Stellar Physics from High-Precision Photometry – Aug 27, a NEW STELLAR.
Scientific aspects of SONG Jørgen Christensen-Dalsgaard Department of Physics and Astronomy Aarhus University.
Photometric detection of the starlight reflection by a “Pegasi” planet Martin Vannier (1), Tristan Guillot (2), Suzanne Aigrain (1) (1) ESO, Chile (2)
Travis Metcalfe (NCAR) Asteroseismology with the Kepler Mission We are the stars which sing, We sing with our light; We are the birds of fire, We fly over.
A Practical Introduction to Stellar Nonradial Oscillations (i) Rich Townsend University of Delaware ESO Chile ̶ November 2006 TexPoint fonts used in EMF.
Extrasolar Planets and Stellar Oscillations in K Giant Stars Notes can be downloaded from
A Dedicated Search for Transiting Extrasolar Planets using a Doppler Survey and Photometric Follow-up A Proposal for NASA's Research Opportunities in Space.
Stellar Activity in the Kepler Era Tom Ayres (CASA)
Travis Metcalfe Space Science Institute + Stellar Astrophysics Centre Asteroseismic Signatures of Magnetic Activity Variations in Solar-type Stars Collaborators:
The Sun as a whole: activity as seen by helioseismology
Time series analysis methods in vivo and silico Nigul Olspert Aalto University ICS
Jim Fuller Caltech/KITP ACOUSTIC OSCILLATIONS IN RED GIANTS.
Precision stellar physics from the ground Andrzej Pigulski University of Wrocław, Poland Special Session #13: High-precision tests of stellar physics from.
A Non-Radial Oscillation Model for Radio Pulsars In collaboration with Dr. J. Christopher Clemens University of North Carolina at Chapel Hill.
The Sun as whole: activity as seen by helioseismology A.C. Birch (Max Planck Institute for Solar System Research)
Constraints on the radial differential rotation of six Sun-like stars Martin Bo Nielsen Laurent Gizon, Hannah Schunker and Jesper Schou Institute for Astrophysics.
Corot Week 61 Targets selection Be stars Paris-Meudon Observatory: A.-M. Hubert, M. Floquet, C. Neiner Univ. of Valencia: J. Fabregat, J. Gutierrez-Soto,
Travis Metcalfe Space Science Institute + Stellar Astrophysics Centre Probing Stellar Activity with Kepler.
Oscillation spectra with regular patterns
Asteroseismology with A-STEP The sun from the South Pole Grec, Fossat & Pomerantz, 1980, Nature, 288, 541.
Travis Metcalfe (NCAR) First results from the Asteroseismic Modeling Portal Collaborators: Michaël Bazot, Tim Bedding, Alfio Bonanno, Isa Brandão, Bill.
Time/frequency analysis with COROT: what do we want to do? F. Baudin & E. Michel Time/frequency analysis : any method providing an information on the temporal.
Flows and Cycles Large scale flows and stellar magnetic cycles Markus Roth Wiebke Herzberg René Kiefer Ariane Schad Guy Davis (UoB) Retreat of the Stellar.
PLAnetary Transits and Oscillations of stars Claude CATALA Observatoire de Paris, LESIA Main Science Requirements.
Thomas Hackman: Stellar differential rotation1 Detecting stellar differential rotation NORDITA – Solar and stellar dynamo cycles Thomas Hackman,
Asteroseismology of Sun-like Stars
2nd CoRoT Brazil Workshop REPORT ON THE Second CoRoT Brazil Workshop (Ubatuba, 2-6th November) 9th CoRoT Week.
AFS Lecture 4. COROT, COnvection, ROtation & Transits exoplanétaires.
Asteroseismology of Kepler
Asteroseismic Modeling Portal (AMP) Development
COROT, COnvection, ROtation & Transits exoplanétaires
Southern HK project Small telescopes at CTIO run by SMARTS partners: Yale, GSU, STScI, et al. Service observing 2-3x per month using RC Spec with R.
Pre-Cursor Data Needed for JWST Transit and Eclipse Observations
Kuhn - HMI Science Interests: Limb photometry and astrometry
Quasi-periodic pulsations in stellar flares observed with XMM-Newton
Strategies to detect Earth-like planets around nearby stars
Corot Be stars group Be stars: The team:
ASTEROSEISMOLOGY OF LATE STAGES OF STELLAR EVOLUTION
Solar-like oscillations with HARPS …and SOPHIE
The SMARTS Southern HK Project
Something New About Frequency Shifts
Goal: Understand cycles in Sunspot frequency over time.
Presentation transcript:

Magnetic activity of F stars Savita Mathur Space Science Institute

Magnetic activity: photometry VIRGO/SPM VIRGO/SPM Sunspot number Red: cross-correlation Black: individual modes WITH RADIO FLUX [Mathur et al. 2013] [García et al. 2010] [Salabert et al. 2009] APS colloquium 2014

The CoRoT target: HD49933 Stellar parameters: F5V dwarf 1.2 M; 1.3 R Observed by CoRoT during 60 + 137 days + 90 days 50 oscillation modes measured Prot = 3.4 days // [Appourchaux et al. 2008; Benomar et al. 2009] APS colloquium 2014

Hints of a magnetic-activity cycle HD49933 Spectroscopy Seismology Red: individual modes Black: cross-correlation Mathur, Metcalfe in prep. [García et al. 2010] Complementary observations Ca HK: Mount Wilson index of 0.31 Active star Anticorrelation between amplitude variation and frequency shifts Pcyc>120days APS colloquium 2014

Coming back to surface rotation Prot<12d HD49933 S-K is jut the star above 1.4M [Garcia et al. in preparation] [García et al. in prep.] APS colloquium 2014

Results: Kepler Shere-Khan Prot=2.5d <Sph> = 250 ppm Asteroseismology: M~1.4M DCZ~3% We observe: Magnetic Cycle-like behaviour Long-lived active longitudes during maximum activity RV measurement at Mercator does not show signature of close binary [Mathur et al. 2014, in press] APS colloquium 2014