CXOU J181852.0-150213 , the SIMBAD biblio

CXOU J181852.0-150213 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.04CEST04:12:49


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Title First 3 Authors
2006ApJ...652L..45R 1 6 17 A new young galactic supernova remnant containing a compact object: G15.9+0.2. REYNOLDS S.P., BORKOWSKI K.J., HWANG U., et al.
2009ApJ...696.1792E 303     A D     X C       8 23 2 Hard X-ray flux upper limits of central compact objects in supernova remnants. ERDEVE I., KALEMCI E. and ALPAR M.A.
2009ARep...53..472M 17 0 The pulsar J1852+0040 in Kes 79 and the nature of central compact objects in supernova remnants. MALOV I.F.
2010ApJ...709..436H 18       D               1 21 158 Spin-down measurement of PSR J1852+0040 in Kesteven 79: central compact objects as anti-magnetars. HALPERN J.P. and GOTTHELF E.V.
2011AJ....142...47P 77             C       1 80 26 The MIPSGAL view of supernova remnants in the galactic plane. PINHEIRO GONCALVES D., NORIEGA-CRESPO A., PALADINI R., et al.
2013ApJ...765...58G 18       D               1 29 138 The spin-down of PSR J0821-4300 and PSR J1210-5226: confirmation of central compact objects as anti-magnetars. GOTTHELF E.V., HALPERN J.P. and ALFORD J.
2016A&A...592L..12K 764           X         19 5 8 Study of a new central compact object: The neutron star in the supernova remnant G15.9+0.2. KLOCHKOV D., SULEIMANOV V., SASAKI M., et al.
2017A&A...597A..65M         O           34 4 Fe K and ejecta emission in SNR G15.9+0.2 with XMM-Newton. MAGGI P. and ACERO F.
2017ApJ...844...84H 42           X         1 33 48 Comparing neutron star kicks to supernova remnant asymmetries. HOLLAND-ASHFORD T., LOPEZ L.A., AUCHETTL K., et al.
2018A&A...609A..74P 85             C       1 7 21 Magnetic neutron star cooling and microphysics. POTEKHIN A.Y. and CHABRIER G.
2018MNRAS.479.3033S 148     A     X         4 4 2 Infrared and X-ray study of the Galactic SNR G15.9+0.2. SASAKI M., MAKELA M.M., KLOCHKOV D., et al.
2019MNRAS.483...70C 42           X         1 97 7 A catalogue of Galactic supernova remnants in the far-infrared: revealing ejecta dust in pulsar wind nebulae. CHAWNER H., MARSH K., MATSUURA M., et al.
2019PASP..131k4301T 42           X         1 11 ~ The kinematic distances of SNR g16.7+0.1 and g15.9+0.2 by analyzing H I absorption spectra. TIAN W.W., ZHU H., ZHANG M.F., et al.
2020MNRAS.491.1585H 43           X         1 30 ~ X-ray spectral analysis of the neutron star in SNR 1E 0102.2-7219. HEBBAR P.R., HEINKE C.O. and HO W.C.G.
2020MNRAS.495.1692G 17       D               1 21 ~ Powering central compact objects with a tangled crustal magnetic field. GOURGOULIATOS K.N., HOLLERBACH R. and IGOSHEV A.P.
2020MNRAS.496.5052P 102       D     X         3 114 60 Thermal luminosities of cooling neutron stars. POTEKHIN A.Y., ZYUZIN D.A., YAKOVLEV D.G., et al.
2021A&A...651A..40M 148       D   O X         4 50 10 A kinematic study of central compact objects and their host supernova remnants. MAYER M.G.F. and BECKER W.
2021RAA....21..294W 670       D     X C       15 16 3 What causes the absence of pulsations in Central Compact Objects in supernova remnants? WU Q., PIRES A.M., SCHWOPE A., et al.
2023ApJ...944...36A 19       D               3 24 3 Do Central Compact Objects have Carbon Atmospheres? ALFORD J.A.J. and HALPERN J.P.

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