%0 Generic %1 beck2015ionized %A Beck, Sara C. %A Turner, Jean L. %A Lacy, John %A Greathouse, Thomas %D 2015 %K formation gas kinematics star %T Ionized Gas Kinematics at High Resolution V: NeII, Multiple Clusters, High Efficiency Star Formation and Blue Flows in He 2-10 %U http://arxiv.org/abs/1510.01742 %X We measured the $12.8\mu$m NeII line in the dwarf starburst galaxy He 2-10 with the high-resolution spectrometer TeXeS on the NASA IRTF. The data cube has diffraction-limited spatial resolution $\sim1^\prime\prime$ and total velocity resolution including thermal broadening of $\sim5$km/s. This makes it possible to compare the kinematics of individual star-forming clumps and molecular clouds in the three dimensions of space and velocity, and allows us to determine star formation efficiencies. The kinematics of the ionized gas confirm that the starburst contains multiple dense clusters. From the $M/R$ of the clusters and the $\simeq30-40$% star formation efficiencies the clusters are likely to be bound and long lived, like globulars. Non-gravitational features in the line profiles show how the ionized gas flows through the ambient molecular material, as well as a narrow velocity feature which we identify with the interface of the HII region and a cold dense clump. These data offer an unprecedented view of the interaction of embedded HII regions with their environment.

@misc{beck2015ionized, abstract = {We measured the $12.8\mu$m [NeII] line in the dwarf starburst galaxy He 2-10 with the high-resolution spectrometer TeXeS on the NASA IRTF. The data cube has diffraction-limited spatial resolution $\sim1^{\prime\prime}$ and total velocity resolution including thermal broadening of $\sim5$km/s. This makes it possible to compare the kinematics of individual star-forming clumps and molecular clouds in the three dimensions of space and velocity, and allows us to determine star formation efficiencies. The kinematics of the ionized gas confirm that the starburst contains multiple dense clusters. From the $M/R$ of the clusters and the $\simeq30-40$% star formation efficiencies the clusters are likely to be bound and long lived, like globulars. Non-gravitational features in the line profiles show how the ionized gas flows through the ambient molecular material, as well as a narrow velocity feature which we identify with the interface of the HII region and a cold dense clump. These data offer an unprecedented view of the interaction of embedded HII regions with their environment.}, added-at = {2015-10-08T10:22:25.000+0200}, author = {Beck, Sara C. and Turner, Jean L. and Lacy, John and Greathouse, Thomas}, biburl = {https://www.bibsonomy.org/bibtex/223fe9662d1588015d9d326d6432a4a8a/miki}, description = {[1510.01742] Ionized Gas Kinematics at High Resolution V: [NeII], Multiple Clusters, High Efficiency Star Formation and Blue Flows in He 2-10}, interhash = {d08f02ab813dd336b78613d719479f22}, intrahash = {23fe9662d1588015d9d326d6432a4a8a}, keywords = {formation gas kinematics star}, note = {cite arxiv:1510.01742Comment: accepted to ApJ}, timestamp = {2015-10-08T10:22:25.000+0200}, title = {Ionized Gas Kinematics at High Resolution V: [NeII], Multiple Clusters, High Efficiency Star Formation and Blue Flows in He 2-10}, url = {http://arxiv.org/abs/1510.01742}, year = 2015 }