We propose a detailed study of the acceleration of particles in the south-westrim of SN 1006 to determine the geometry of the acceleration in this prototypeof the class of radio bipolar supernova remnants. To reach our goal, we need tocharacterize the following quantities in both synchrotron rims all along theshock at the scale of the width of the synchrotron filaments: cut-off frequencyof the synchrotron spectrum and downstream magnetic field, together withestimates of the level of spectral and hydrodynamical back-reaction. Ourprevious LP on SN 1006 provides these quantities for the north-east rim, but notfor the south-west rim which hence has insufficient statistics. To achieve theabove objectives, we need a new observation of 120 ks of the south-west rim.
Publications
XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration |Miceli, M., Bocchino, F., et al. | A&A | 546-66 | 2012 | 2012A&A...546A..66M | http://ui.adsabs.harvard.edu/#abs/2012A&A...546A..66M
The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton |Miceli, M., Bocchino, F., et al. | A&A | 556-80 | 2013 | 2013A&A...556A..80M | http://ui.adsabs.harvard.edu/#abs/2013A&A...556A..80M
The loss-limited electron energy in SN 1006: Effects of the shock velocity and of the diffusion process |Miceli, M., Bocchino, F., et al. | AN | 335-252 | 2014 | 2014AN....335..252M | http://ui.adsabs.harvard.edu/#abs/2014AN....335..252M
XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy |Li, Jiang-Tao, Decourchelle, Anne, et al. | MNRAS | 453-3953 | 2015 | 2015MNRAS.453.3953L | http://ui.adsabs.harvard.edu/#abs/2015MNRAS.453.3953L
Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and gamma-ray emission |Miceli, M., Orlando, S., et al. | A&A | 593-26 | 2016 | 2016A&A...593A..26M | http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..26M
Detection of Two TeV Shell-type Remnants at GeV Energies with FERMI LAT: HESS J1731-347 and SN 1006 |Condon, B., Lemoine-Goumard, M., et al. | ApJ | 851-100 | 2017 | 2017ApJ...851..100C | http://ui.adsabs.harvard.edu/#abs/2017ApJ...851..100C
Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006 |Li, Jiang-Tao, Ballet, Jean, et al. | ApJ | 864-85 | 2018 | 2018ApJ...864...85L | http://ui.adsabs.harvard.edu/#abs/2018ApJ...864...85L
Genus Statistic Applied to the X-Ray Remnant of SN 1572: Clues to the Clumpy Ejecta Structure of Type Ia Supernovae |Sato, Toshiki, Hughes, John P., et al. | ApJ | 879-64 | 2019 | 2019ApJ...879...64S | http://ui.adsabs.harvard.edu/#abs/2019ApJ...879...64S
Fermi LAT detection of the supernova remnant SN 1006 revisited: The southwest limb |Xing, Yi, Wang, Zhongxiang, et al. | PASJ | 71-77 | 2019 | 2019PASJ...71...77X | http://ui.adsabs.harvard.edu/#abs/2019PASJ...71...77X
Erratum: .XMM-newton large program on SN1006 - II: Thermal emission. (2016, MNRAS, 462, 158) |Li, Jiang-Tao, Decourchelle, Anne, et al. | MNRAS | 499-862 | 2020 | 2020MNRAS.499..862L | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499..862L
Erratum: XMM-Newton large program on SN1006 - I. Methods and initial results of spatially resolved spectroscopy |Li, Jiang-Tao, Decourchelle, Anne, et al. | MNRAS | 499-5679 | 2020 | 2020MNRAS.499.5679L | http://ui.adsabs.harvard.edu/#abs/2020MNRAS.499.5679L
Modeling particle acceleration and non-thermal emission in supernova remnants |Orlando, S., Miceli, M., et al. | NewA | 86-101566 | 2021 | 2021NewA...8601566O | http://ui.adsabs.harvard.edu/#abs/2021NewA...8601566O
Indication of a fast ejecta fragment in the atomic cloud interacting with the southwestern limb of SN 1006 |Giuffrida, R., Miceli, M., et al. | A&A | 684-A68 | 2024 | 2024A&A...684A..68G | http://ui.adsabs.harvard.edu/#abs/2024A&A...684A..68G
Instrument
EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage
2010-08-28T00:39:12Z/2010-08-29T12:47:02Z
Version
17.56_20190403_1200
Mission Description
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Dr Anne Decourchelle, 2011, 'Geometry of the acceleration in the bipolar supernova remnant of SN 1006', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rl7ndhb
