Academic Journal
ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7
| العنوان: | ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 |
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| المؤلفون: | Strandet, M. L., Weiss, A., Breuck, C. De, Marrone, D. P., Vieira, J. D., Aravena, M., Ashby, M. L. N., Béthermin, M., Bothwell, M. S., Bradford, C. M., Carlstrom, J. E., Chapman, S. C., Cunningham, D. J. M., Chen, Chian-Chou, Fassnacht, C. D., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hayward, C. C., Hezaveh, Y., Litke, K., Ma, J., Malkan, M., Menten, K. M., Miller, T., Murphy, E. J., Narayanan, D., Phadke, K. A., Rotermund, K. M., Spilker, J. S., Sreevani, J. |
| Thesis Advisors: | Univ Arizona, Steward Observ |
| بيانات النشر: | IOP PUBLISHING LTD, 2017. |
| سنة النشر: | 2017 |
| المجموعة: | University of Arizona |
| Original Material: | ISM Properties of a Massive Dusty Star-forming Galaxy Discovered at z ∼ 7 2017, 842 (2):L15 The Astrophysical Journal The Astrophysical Journal Letters |
| مصطلحات موضوعية: | early universe, galaxies: high-redshift, galaxies: star formation |
| الوصف: | We report the discovery and constrain the physical conditions of the interstellar medium of the highest-redshift millimeter-selected dusty star-forming galaxy to date, SPT-S J031132-5823.4 (hereafter SPT0311-58), at z = 6.900 +/- 0.002. SPT0311-58 was discovered via its 1.4 mm thermal dust continuum emission in the South Pole Telescope (SPT)-SZ survey. The spectroscopic redshift was determined through an Atacama Large Millimeter/submillimeter Array 3 mm frequency scan that detected CO(6-5), CO(7-6), and [C I](2-1), and subsequently was confirmed by detections of CO(3-2) with the Australia Telescope Compact Array and[C II] with APEX. We constrain the properties of the ISM in SPT0311-58 with a radiative transfer analysis of the dust continuum photometry and the CO and [C I] line emission. This allows us to determine the gas content without ad hoc assumptions about gas mass scaling factors. SPT0311-58 is extremely massive, with an intrinsic gas mass of M-gas = 3.3 +/- 1.9 x 10(11) M-circle dot. Its large mass and intense star formation is very rare for a source well into the epoch of reionization. |
| Original Identifier: | oai:arizona.openrepository.com:10150/627112 |
| نوع الوثيقة: | Article |
| اللغة: | English |
| تدمد: | 2041-8213 |
| Relation: | http://stacks.iop.org/2041-8205/842/i=2/a=L15?key=crossref.2889705e08884104c5e080d3961c07ae |
| DOI: | 10.3847/2041-8213/aa74b0 |
| الاتاحة: | http://hdl.handle.net/10150/627112 http://arizona.openrepository.com/arizona/handle/10150/627112 |
| Rights: | © 2017. The American Astronomical Society. All rights reserved. |
| رقم الانضمام: | edsndl.arizona.edu.oai.arizona.openrepository.com.10150.627112 |
| قاعدة البيانات: | Networked Digital Library of Theses & Dissertations |
Full Text Finder | تدمد: | 20418213 |
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| DOI: | 10.3847/2041-8213/aa74b0 |