ALMA Polarimetry of AT2018cow
暂无分享,去创建一个
Y. Urata | K. Asada | K. Yamaoka | K. Toma | M. Tashiro | G. Petitpas | H. Nagai | S. Takahashi | Satoko Takahashi | K. Huang | Kuiyun Huang | J. Shimoda | G. Petitpas
[1] N. Kanekar,et al. H i 21 cm mapping of the host galaxy of AT2018cow: a fast-evolving luminous transient within a ring of high column density gas , 2019, Monthly Notices of the Royal Astronomical Society: Letters.
[2] M. Lyutikov,et al. Fast-rising blue optical transients and AT2018cow following electron-capture collapse of merged white dwarfs , 2018, Monthly Notices of the Royal Astronomical Society.
[3] N. Soker,et al. Diversity of common envelope jets supernovae and the fast transient AT2018cow , 2018, Monthly Notices of the Royal Astronomical Society.
[4] E. Phinney,et al. AT2018cow: A Luminous Millimeter Transient , 2018, The Astrophysical Journal.
[5] C. Guidorzi,et al. An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients , 2018, The Astrophysical Journal.
[6] P. Brown,et al. Swift spectra of AT2018cow: a white dwarf tidal disruption event? , 2018, Monthly Notices of the Royal Astronomical Society.
[7] William H. Lee,et al. The fast, luminous ultraviolet transient AT2018cow: extreme supernova, or disruption of a star by an intermediate-mass black hole? , 2018, Monthly Notices of the Royal Astronomical Society.
[8] A. Lazarian,et al. Discovery of Kolmogorov-like magnetic energy spectrum in Tycho’s supernova remnant by two-point correlations of synchrotron intensity , 2018, Monthly Notices of the Royal Astronomical Society.
[9] P. Brown,et al. X-ray Swift observations of SN 2018cow , 2018, Monthly Notices of the Royal Astronomical Society: Letters.
[10] B. J. Shappee,et al. The Cow: Discovery of a Luminous, Hot, and Rapidly Evolving Transient , 2018, The Astrophysical Journal.
[11] R. Indebetouw,et al. Detection of Linear Polarization in the Radio Remnant of Supernova 1987A , 2018, The Astrophysical Journal.
[12] Tsuyoshi Inoue,et al. THE ORIGIN OF RADIALLY ALIGNED MAGNETIC FIELDS IN YOUNG SUPERNOVA REMNANTS , 2013, 1305.4656.
[13] John P. Hughes,et al. ON THE RADIO POLARIZATION SIGNATURE OF EFFICIENT AND INEFFICIENT PARTICLE ACCELERATION IN SUPERNOVA REMNANT SN 1006 , 2013, 1302.4678.
[14] K. Institute,et al. Faraday rotation measure synthesis , 2005, astro-ph/0507349.
[15] M. Wolleben,et al. The Magnetic Field of the Large Magellanic Cloud Revealed Through Faraday Rotation , 2005, Science.
[16] M. Rupen,et al. SN 1993J VLBI. III. The Evolution of the Radio Shell , 2003, astro-ph/0307382.
[17] J. Dickel,et al. Radio Spectral Index Variations and Physical Conditions in Kepler’s Supernova Remnant , 2002, astro-ph/0210355.
[18] R. Chevalier. Synchrotron Self-Absorption in Radio Supernovae , 1998 .
[19] D. Palmer,et al. BATSE observations of gamma-ray burst spectra. I: Spectral diversity , 1993 .
[20] W. V. Breugel,et al. Radio structure of the remnant of Tycho's supernova (SN 1572) , 1991 .
[21] D. Milne,et al. An atlas of supernova remnant magnetic fields , 1988 .
[22] A. Bell. The acceleration of cosmic rays in shock fronts – I , 1978 .
[23] Jeremiah P. Ostriker,et al. Particle Acceleration by Astrophysical Shocks , 1978 .
[24] J. R. Jokipii. COSMIC-RAY PROPAGATION. I. CHARGED PARTICLES IN A RANDOM MAGNETIC FIELD. , 1966 .