• Massive Star Formation: Accreting from Companion

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      https://www.ias.ac.in/article/fulltext/joaa/035/03/0495-0496

    • Keywords

       

      Infrared: ISM; stars: formation; ISM: jets and outflows.

    • Abstract

       

      We report the possible accretion from companion in the massive star forming region (G350.69–0.49). This region seems to be a binary system composed of a diffuse object (possible nebulae or UC HII region) and a Massive Young Stellar Object (MYSO) seen in Spitzer IRAC image. The diffuse object and MYSO are connected by the shock-excited 4.5 𝜇m emission, suggesting that the massive star may form through accreting material from the companion in this system.

    • Author Affiliations

       

      X. Chen1 J. S. Zhang2

      1. Key Laboratory for Research in Galaxies and Cosmology, Key Laboratory of Radio Astronomy, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China.
      2. Centre for Astrophysics, Guangzhou University, Guangzhou 510006, China.
    • Dates

       
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