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        <dc:title>A glimpse of the Southern Jellyfish Nebula and its massive YSO</dc:title>
        <dc:creator>Mercer, EP</dc:creator>
        <dc:creator>Wolff, MJ</dc:creator>
        <dc:creator>Bania, TM</dc:creator>
        <dc:creator>Benjamin, RA</dc:creator>
        <dc:creator>Cohen, M</dc:creator>
        <dc:creator>Dickey, JM</dc:creator>
        <dc:creator>Jackson, JM</dc:creator>
        <dc:creator>Kobulnicky, HA</dc:creator>
        <dc:creator>Mathis, JS</dc:creator>
        <dc:creator>Stolovy, SR</dc:creator>
        <dc:creator>Uzpen, B</dc:creator>
        <dc:creator>Clemens, DP</dc:creator>
        <dc:creator>Churchwell, EB</dc:creator>
        <dc:creator>Rathborne, JM</dc:creator>
        <dc:creator>Meade, MR</dc:creator>
        <dc:creator>Babler, BL</dc:creator>
        <dc:creator>Indebetouw, R</dc:creator>
        <dc:creator>Whitney, BA</dc:creator>
        <dc:creator>Watson, C</dc:creator>
        <dc:creator>Wolfire, MG</dc:creator>
        <dc:subject>240101 Astronomy and Astrophysics</dc:subject>
        <dc:description>In Spitzer/IRAC images obtained under the GLIMPSE Legacy Survey, we have identified a unique and provocative&#13;
nebular object we call the ‘‘Southern Jellyfish Nebula.’’ The Southern Jellyfish Nebula is characterized by&#13;
a fan of narrow tendrils with extreme length-to-width ratios that emanate from the vicinity of a bright infrared point&#13;
source embedded in a smaller resolved nebula. From CO observations of the Nebula’s morphologically associated&#13;
molecular cloud, we have derived a kinematic distance of 5:7  0:8 kpc and a cloud mass of 3:2  0:9 ; 103 M. The&#13;
tendril-like ropes of the Nebula have widths of 0.1 pc and lengths of up to 2 pc. We have integrated the infrared&#13;
spectral energy distribution (SED) of the point source to establish it as a massive young stellar object (MYSO), most&#13;
likely forming alone, but possibly masking fainter cluster members. The shape of the SED is consistent with the shape&#13;
of a late Class 0 SED model. Based on its far-IR luminosity of 3:3  0:9 ; 104 L, the Southern Jellyfish’sMYSO has&#13;
a zero-age main sequence (ZAMS) spectral type of B0. Given the curious nature of this nebula, we suspect its peculiar&#13;
IR-bright structure is directly related to its current state of star formation.</dc:description>
        <dc:publisher>University of Chicago Press</dc:publisher>
        <dc:date>2007</dc:date>
        <dc:type>Article</dc:type>
        <dc:type>PeerReviewed</dc:type>
        <dc:format>application/pdf</dc:format>
        <dc:identifier>http://eprints.utas.edu.au/4098/1/4098.pdf</dc:identifier>
        <dc:relation>http://dx.doi.org/10.1086/510302</dc:relation>
        <dc:identifier>Mercer, EP and Wolff, MJ and Bania, TM and Benjamin, RA and Cohen, M and Dickey, JM and Jackson, JM and Kobulnicky, HA and Mathis, JS and Stolovy, SR and Uzpen, B and Clemens, DP and Churchwell, EB and Rathborne, JM and Meade, MR and Babler, BL and Indebetouw, R and Whitney, BA and Watson, C and Wolfire, MG (2007) A glimpse of the Southern Jellyfish Nebula and its massive YSO. The Astrophysical Journal, 656 (1). pp. 242-247. ISSN 0004-637X</dc:identifier>
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