Multiple Outflows Traced by H2O Masers around the Ultra-Compact H II Region G 34.26+0.15

DOI PDF 被引用文献6件
  • Hiroshi Imai
    1Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065 hiroimai@sci.kagoshima-u.ac.jp
  • Rui Omi
    2Department of Physics, Faculty of Science, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065
  • Tomoharu Kurayama
    1Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065 hiroimai@sci.kagoshima-u.ac.jp
  • Takumi Nagayama
    1Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065 hiroimai@sci.kagoshima-u.ac.jp
  • Tomoya Hirota
    3Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
  • Takeshi Miyaji
    3Mizusawa VLBI Observatory, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588
  • Toshihiro Omodaka
    1Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima, Kagoshima 890-0065 hiroimai@sci.kagoshima-u.ac.jp

書誌事項

公開日
2011-12-25
DOI
  • 10.1093/pasj/63.6.1293
公開者
Oxford University Press (OUP)

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<jats:title>Abstract</jats:title> <jats:p>We present the results of VLBI observations of the H$_2$O masers associated with the massive-star forming region G 34.26$+$0.15 with the Very Long Baseline Array (VLBA), the Japanese VLBI Network (JVN), and the VLBI Exploration of Radio Astrometry (VERA) to reveal the whole three-dimensional kinematical structure of the H$_2$O maser region (2$''$$\times$ 5$''$). From the result of one of the astrometric observations with VERA and the revealed maser distribution, we found that, in G 34.26$+$0.15, the H$_2$O masers are likely to be associated with four young stellar objects (YSOs), each of which is traced by at least one of millimeter-continuum and molecular-line emission peaks, rather than by centimeter-continuum peaks that may trace H II regions, including the brightest millimeter- and centimeter-continuum emission peak. We also measured the relative proper motions of 33 H$_2$O masers in the VLBA observations (1996 December–1997 May) and 104 ones in JVN/VERA (2006 March–2008 June). We found that these maser motions indicate large random motion (40–70 km s$^{-1}$), but in at least one region they exhibit radial expansion motions. This suggests the existence of outflows originating from accompanying YSOs. We discuss not only the intrinsic physical properties of multiple YSOs that harbor H$_2$O masers within 0.1 pc but also the implications of the existence of these YSOs. The formation history of the cometary H II region in G 34.26$+$0.15 is also discussed.</jats:p>

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