Jet-induced Enhancement of the Nova Rate in M87

Massimo Della Valle, Allen W. Shafter and Sumner Starrfield
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Abstract

We argue that the Bondi accretion mechanism has the potential to enhance classical nova production near the M87 jet. According to our estimates, the jet's influence can increase the nova rate in its vicinity by up to a factor of two over the background rate by triggering explosions on single white dwarfs. This result may offer a straightforward explanation for the recently observed excess of novae near the M87 jet.
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射流诱发的 M87 新星率增强
我们认为邦迪吸积机制有可能增强M87喷流附近的经典新星生成。根据我们的估算,喷流的影响可以通过触发单个白矮星的爆炸,将其附近的新星率提高到背景率的两倍。这一结果可以直接解释最近观测到的M87喷流附近新星过多的现象。
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