ALMA Observations of HCO+ and HCN Emission in the Massive Star-forming Region N55 of the Large Magellanic Cloud
| العنوان: | ALMA Observations of HCO+ and HCN Emission in the Massive Star-forming Region N55 of the Large Magellanic Cloud |
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| المؤلفون: | A. J. Nayana, T. Onishi, N. Naslim, M. Galametz, Salah Nasri, Kazuki Tokuda, S. C. Madden, O. Morata, Francisca Kemper |
| المصدر: | The Astrophysical Journal. 902:140 |
| بيانات النشر: | American Astronomical Society, 2020. |
| سنة النشر: | 2020 |
| مصطلحات موضوعية: | Physics, Star formation, Resolution (electron density), FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, Star (graph theory), Astrophysics - Astrophysics of Galaxies, Galaxy, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Protostar, Large Magellanic Cloud, Image resolution, Stellar evolution |
| الوصف: | We present the results of high spatial resolution HCO$^{+}$($1-0$) and HCN($1-0$) observations of N55 south region (N55-S) in the Large Magellanic Cloud (LMC), obtained with the Atacama Large Millimeter/submillimeter Array (ALMA). N55-S is a relatively less extreme star-forming region of the LMC characterized by a low radiation field. We carried out a detailed analysis of the molecular emission to investigate the relation between dense molecular clumps and star formation in the quiescent environment of N55-S. We detect ten molecular clumps with significant HCO$^{+}(1-0)$ emission and eight with significant HCN($1-0$) emission, and estimate the molecular clump masses by virial and local thermodynamic equilibrium analysis. All identified young stellar objects (YSOs) in the N55-S are found to be near the HCO$^{+}$ and HCN emission peaks showing the association of these clumps with recent star formation activity. The molecular clumps that have associated YSOs show relatively larger linewidths and masses than those without YSOs. We compare the clump properties of the N55-S with those of other giant molecular clouds (GMCs) in the LMC and find that N55-S clumps possess similar size but relatively lower linewidth and larger HCN/HCO$^{+}$(1$-$0) flux ratio. These results can be attributed to the low radiation field in N55-S resulted by relatively low star formation activity compared to other active star-forming regions like 30Doradus-10 and N159. The dense gas fraction of N55-S is $\sim$ 0.025, lower compared to other GMCs of the LMC supporting the low star formation efficiency of this region. Accepted for publication in ApJ, 13 pages, 4 figures |
| تدمد: | 1538-4357 0004-637X |
| URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_dedup___::34db8ca1714eb3031934b171822878b0 https://doi.org/10.3847/1538-4357/abb466 |
| حقوق: | OPEN |
| رقم الأكسشن: | edsair.doi.dedup.....34db8ca1714eb3031934b171822878b0 |
| قاعدة البيانات: | OpenAIRE |
| تدمد: | 15384357 0004637X |
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