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首页> 外文期刊>The Astrophysical journal >ADAPTIVE OPTICS DISCOVERY OF SUPERNOVA 2004ip IN THE NUCLEAR REGIONS OF THE LUMINOUS INFRARED GALAXY IRAS 18293-3413
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ADAPTIVE OPTICS DISCOVERY OF SUPERNOVA 2004ip IN THE NUCLEAR REGIONS OF THE LUMINOUS INFRARED GALAXY IRAS 18293-3413

机译:红外红外星空IRAS 18293-3413核区中超新星2004ip的自适应光学发现

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We report a supernova discovery in K_s-band images from the NAOS CONICA adaptive optics (AO) system on the ESO Very Large Telescope. The images were obtained as part of a near-infrared search for highly obscured supernovae in the nuclear regions of luminous and ultraluminous infrared galaxies. SN 2004ip is located within a circumnuclear starburst at 1.4″ (or 500 pc) projected distance from the K-band nucleus of the luminous infrared galaxy IRAS 18293 - 3413. The supernova luminosity and light curve are consistent with a core-collapse event suffering from a host galaxy extinction of up to about 40 mag in the V band, which is as expected for a circumnuclear starburst environment. This is the first supernova to be discovered making use of AO correction and demonstrates the potential of the current 8 m-class telescopes equipped with AO in discovering supernovae from the innermost nuclear regions of luminous and ultraluminous infrared galaxies.
机译:我们在ESO超大型望远镜的NAOS CONICA自适应光学(AO)系统的K_s波段图像中报告了超新星发现。这些图像是作为近红外搜索的一部分而获得的,该搜索是在发光和超发光红外星系的核区中高度模糊的超新星。 SN 2004ip位于离核红外星系IRAS 18293-3413的K带原子核投影距离为1.4“(或500 pc)的外核爆炸中。超新星的光度和光度曲线与遭受核坍塌事件的影响一致V波段高达约40 mag的主星系消光,这在周围核星爆环境中是预期的。这是利用AO校正技术发现的第一个超新星,并展示了当前配备AO的8 m级望远镜在从发光和超发光红外星系的最内核区域发现超新星的潜力。

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