تقرير
ALMA Observation of NGC5135: The Circumnuclear CO(6-5) and Dust Continuum Emission at 45 Parsec Resolution[$\star$]
العنوان: | ALMA Observation of NGC5135: The Circumnuclear CO(6-5) and Dust Continuum Emission at 45 Parsec Resolution[$\star$] |
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المؤلفون: | Cao, Tianwen, Lu, Nanyao, Xu, C. Kevin, Zhao, Yinghe, Kalari, Venu Madhav, Gao, Yu, Charmandaris, Vassilis, Santos, Tanio Diaz, van der Werf, Paul, Cao, Chen, Wu, Hong, Inami, Hanae, Evans, Aaron |
سنة النشر: | 2018 |
المجموعة: | Astrophysics |
مصطلحات موضوعية: | Astrophysics - Astrophysics of Galaxies |
الوصف: | We present high-resolution (0.17\arcsec $\times$ 0.14\arcsec) Atacama Large Millimeter/submillimeter Array (ALMA) observations of the CO\,(6-5) line, and 435\um\ dust continuum emission within a $\sim$9\arcsec $\times$ 9\arcsec\ area centered on the nucleus of the galaxy NGC\,5135. NGC\,5135 is a well-studied luminous infrared galaxy that also harbors a Compton-thick active galactic nucleus (AGN). At the achieved resolution of 48 $\times$ 40\,pc, the CO\,(6-5) and dust emissions are resolved into gas "clumps" along the symmetrical dust lanes associated with the inner stellar bar. The clumps have radii between $\sim$45-180\,pc and CO\,(6-5) line widths of $\sim$60-88\,\kms. The CO\,(6-5) to dust continuum flux ratios vary among the clumps and show an increasing trend with the \FeII/Br-$\gamma$ ratios, which we interpret as evidence for supernova-driven shocked gas providing a significant contribution to the \co65\ emission. The central AGN is undetected in continuum, nor in CO\,(6-5) if its line velocity width is no less than $\sim$\,40\,\kms. We estimate that the AGN contributes at most 1\% of the integrated CO\,(6-5) flux of 512 $\pm$ 24$\,$Jy\kms\ within the ALMA field of view, which in turn accounts for $\sim$32\% of the CO\,(6-5) flux of the whole galaxy. Comment: 21 pages, 12 figures, Accepted for publication in ApJ |
نوع الوثيقة: | Working Paper |
DOI: | 10.3847/1538-4357/aae1f4 |
URL الوصول: | http://arxiv.org/abs/1809.06283 |
رقم الأكسشن: | edsarx.1809.06283 |
قاعدة البيانات: | arXiv |
DOI: | 10.3847/1538-4357/aae1f4 |
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