RESULTS FROM TYCHO SNR CALMEDIUM OBSERVATION

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Presentation transcript:

RESULTS FROM TYCHO SNR CALMEDIUM OBSERVATION Leicester, 07 March 2012 EPIC Calibration Meeting RESULTS FROM TYCHO SNR CALMEDIUM OBSERVATION FABIO GASTALDELLO INAF, IASF-Milano ANDREA TIENGO (IUSS Pavia, IASF-Milano)

New observing mode for guest observer ? MOTIVATIONS Decay of internal calibration source: half-life of Fe55: 2.7 yr meaning that 30 ks in 2000 corresponds to 1.4 Ms in 2015 New observing mode for guest observer ?

SUZAKU RESULTS Furuzawa+09

SUZAKU RESULTS No variation of centroid of Fe line Furuzawa+09 No variation of centroid of Fe line Decreasing FWHM of the line with radius

SUZAKU RESULTS Consistent with shell spherical expansion Furuzawa+09 Consistent with shell spherical expansion Central high FWHM due to blue and redshifted lines

SET OF XMM OBSERVATIONS 3 observations of Tycho SNR: Medium (30/12/07): 17-19-12 ks CALmedium (01/01/08): 46-36-33 ks CALclosed (03/0108): 26-26-22 ks

SPECTRAL MODELING

SPECTRAL MODELING Zero width Free width

SPECTRAL MODELING M1 REG4 (peak of emission) M1 REG6

SPECTRAL MODELING M1 REG1 M2 REG1

RESULTS IN SUZAKU ANNULI CALclosed

RESULTS IN SUZAKU ANNULI CALclosed

RESULTS IN SUZAKU ANNULI Medium

RESULTS IN SUZAKU ANNULI Medium

RESULTS IN SUZAKU ANNULI 12 12 MOS 1 Medium and CALmedium

RESULTS IN SUZAKU ANNULI 12 12 MOS 2 Medium and CALmedium

RESULTS IN SUZAKU ANNULI PN Medium and CALmedium

RESULTS IN SUZAKU ANNULI M1: -9 ± 12 eV M2: 5 ± 24 eV PN: 9 ± 10 eV

RESULTS IN SUZAKU ANNULI M1: 8 ± 5 eV M2: 5 ± 4 eV PN: -2 ± 7 eV

RESULTS IN SUZAKU ANNULI M1: 517 ± 13 eV M2: 529 ± 14 eV PN: 523 ± 11 eV

NEW NRCO ON PERSEUS ? M2 PERSEUS M2 CALCLOSED M2 TYCHO

NEW NRCO ON PERSEUS ?

NEW NRCO ON PERSEUS ?