Anomalous Microwave Emission from Star Forming Regions

<table>L675 star-forming dark cloud. Greyscale shows the anomalous emission on large scales as observed with the AMI telescope [<a href="/journals/aa/2013/390287/#B135">123</a>, <a href="/journals/aa/2013/390287/#B134">125</a>], and white contours show the compact radio emission from the proposed YSO [<a href="/journals/aa/2013/390287/#B132">126</a>, <a href="/journals/aa/2013/390287/#B133">127</a>] with contours at intervals of <svg height="14.9375" id="M221" style="vertical-align:-3.39069pt" version="1.1" viewbox="0 0 37.012501 14.9375" width="37.012501" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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<g transform="matrix(.012,-0,0,-.012,17.825,14.737)"><path d="M181 342h2q63 107 121 107q24 0 41 -16t17 -34q0 -34 -32 -49q-17 -7 -26 2q-21 20 -43 20q-20 0 -42 -22t-38 -63v-183q0 -50 12.5 -62t69.5 -16v-26h-230v26q47 5 58 17t11 61v207q0 49 -9 60.5t-53 16.5v23q74 12 141 40v-109z" id="x72"></path></g><g transform="matrix(.012,-0,0,-.012,22.311,14.737)"><path d="M797 0h-214v26q46 5 58 17.5t12 63.5v167q0 116 -88 116q-48 0 -112 -52q3 -18 3 -42v-195q0 -46 11 -58t53 -17v-26h-214v26q48 5 59.5 17t11.5 60v172q0 115 -88 115q-47 0 -109 -52v-235q0 -47 10 -59.5t48 -17.5v-26h-211v26q50 5 62.5 17t12.5 60v207q0 48 -9 59.5
t-52 18.5v23q79 14 139 41v-81q3 2 29 20.5t44 29.5q45 28 81 28t66 -22t46 -61q25 20 83 57q39 26 76 26q59 0 93 -40t34 -113v-193q0 -49 10.5 -60.5t54.5 -16.5v-26z" id="x6D"></path></g><g transform="matrix(.012,-0,0,-.012,31.973,14.737)"><path d="M319 325l-25 -7q-33 99 -103 99q-29 0 -47 -19.5t-18 -49.5t22 -49.5t62 -36.5q63 -26 95 -57t32 -79q0 -64 -50 -101t-115 -37q-35 0 -67.5 10.5t-46.5 23.5q-5 11 -11 51t-6 67l27 5q14 -53 46.5 -88.5t75.5 -35.5q29 0 50 19.5t21 50.5t-19.5 51.5t-59.5 39.5
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</svg>. The position of the sub-mm peak from 850 <i>μ</i>m data [<a href="/journals/aa/2013/390287/#B154">124</a>] is marked as a red cross.</table>

Advances in Astronomy

Anomalous Microwave Emission from Star Forming Regions

Figure 7