SN 2002cx是一顆奇特的Ia型超新星 [6] [7] [8] 。 它由 勞倫斯伯克利國家實驗室 的研究團隊於2002年5月發現 [ 2 ] 。 它與通常的Ia型超新星不同，於先前發現的幾個奇特Ia型超新星也不同，例如 SN 1991T 和 SN 1991bg [ 5 ] [ 9 ] 。

SN 2002cx是一颗奇特的Ia型超新星 [6] [7] [8] 。 它由 劳伦斯伯克利国家实验室 的研究团队于2002年5月发现 [ 2 ] 。 它与通常的Ia型超新星不同，于先前发现的几个奇特Ia型超新星也不同，例如 SN 1991T 和 SN 1991bg [ 5 ] [ 9 ] 。

We present photometric and spectroscopic observations of supernova (SN) 2002cx, which reveal it to be unique among all observed Type Ia supernovae (SNe Ia). SN 2002cx exhibits an SN 1991T-like premaximum spectrum, an SN 1991bg-like luminosity, and expansion velocities roughly half those of normal SNe Ia. Photometrically, SN 2002cx has a broad peak in the R band and a plateau phase in the I

SN 2002cx exhibits an SN 1991T-like premaximum spectrum, an SN 1991bg-like luminosity, and expansion velocities roughly half those of normal SNe Ia. Photometrically, SN 2002cx has a broad peak in the R band and a plateau phase in the I band, and slow late-time decline. The B-V color evolution is nearly normal, but the V-R and V-I colors are

We present photometric and spectroscopic observations of supernova (SN) 2002cx, which reveal it to be unique among all observed Type Ia supernovae (SNe Ia). SN 2002cx exhibits an SN 1991T-like premaximum spectrum, an SN 1991bg-like luminosity, and expansion velocities roughly half those of normal SNe Ia. Photometrically, SN 2002cx has a broad peak in the R band and a plateau phase in the I

SN 2002cx是一顆奇特的Ia型超新星 [6] [7] [8] 。 它由 勞倫斯伯克利國家實驗室 的研究團隊於2002年5月發現 [ 2 ] 。 它與通常的Ia型超新星不同，於先前發現的幾個奇特Ia型超新星也不同，例如 SN 1991T 和 SN 1991bg [ 5 ] [ 9 ] 。