SNR G007.5-01.7 , the SIMBAD biblio

SNR G007.5-01.7 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST10:41:34


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Title First 3 Authors
2008ApJ...681..320R 625   K A     X C       16 18 9 Discovery of a new X-ray filled radio supernova remnant around the pulsar wind nebula in 3EG J1809-2328. ROBERTS M.S.E. and BROGAN C.L.
2012ApJ...755..151V 217     A     X C       5 4 7 A Chandra proper motion for PSR J1809-2332. VAN ETTEN A., ROMANI R.W. and NG C.-Y.
2013ApJ...775..124F 16       D               1 98 6 Population synthesis of young isolated neutron stars: the effect of fallback disk accretion and magnetic field evolution. FU L. and LI X.-D.
2016MNRAS.463.2932M 80           X         2 16 3 Searching for the optical counterparts of two young γ-ray pulsars. MIGNANI R.P., TESTA V., MARELLI M., et al.
2018ApJ...859...69A 41           X         1 34 4 GeV emission in the region of HESS J1809-193 and HESS J1813-178 is HESS J1809-193 a proton pevatron? ARAYA M.
2018A&A...612A...3H viz 16       D               1 127 45 Population study of Galactic supernova remnants at very high γ-ray energies with H.E.S.S. HESS COLLABORATION, ABDALLA H., ABRAMOWSKI A., et al.
2020MNRAS.493.3159G viz 17       D               1 116 25 Realistic modelling of wind and supernovae shocks in star clusters: addressing 22Ne/20Ne and other problems in Galactic cosmic rays. GUPTA S., NATH B.B., SHARMA P., et al.
2022MNRAS.514.4606I 18       D               1 121 11 Initial periods and magnetic fields of neutron stars. IGOSHEV A.P., FRANTSUZOVA A., GOURGOULIATOS K.N., et al.
2022ApJ...940...63R 18       D               1 224 8 Distances, Radial Distribution, and Total Number of Galactic Supernova Remnants. RANASINGHE S. and LEAHY D.
2023AJ....166..149F 47           X         1 30 ~ EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8-6.3. FILIPOVIC M.D., DAI S., ARBUTINA B., et al.
2023ApJS..268...61Z 47           X         1 249 ~ A Systematic Study of Associations between Supernova Remnants and Molecular Clouds. ZHOU X., SU Y., YANG J., et al.

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