The environment near SNR W41 and W30

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X-rays in the field of W30

•PSR B1800-21/PWN

•Suzaku Source 1:

unresolved; photon index -0.3

favors HMXB explanation.

•Suzaku Source 2:

extended; photon index 1.7 with highly

absorbed column density.

X-ray nature of the LINER nuclear sources

The Evolution & Structure of Pulsar Wind Nebulae

The Interactions between the SNRs and Their Environments

OH maser Suzaku 1 / 2 Thermal X-rays G8.31-0.09 HESS obs PSR… Castro & Slane 2010

X-rays in the field of W30 •PSR B1800-21/PWN •Suzaku Source 1: unresolved; photon index -0.3 favors HMXB explanation. •Suzaku Source 2: extended; photon index 1.7 with highly absorbed column density.

Page 1 and 2: The environment near SNR W41 and W3
Page 3 and 4: W41
Page 5 and 6: XMM-Newton observation 0.3-1.5keV 1
Page 7 and 8: Chandra map Zoom in Misanovic et al
Page 9 and 10: SED of W41 GeV break GeV-TeV break
Page 11: W30 complex •SNR G8.7-0.1 (W30)
Page 15 and 16: GeV break GeV-TeV break
Page 17 and 18: Possible explainations •PWN? high
Page 19 and 20: SNR-MC • One cloud or two clouds?

The environment near SNR W41 and W30

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