dc.creator | Sorai, K. | |
dc.creator | Hasegawa, T. | |
dc.creator | Booth, Roy S. | |
dc.creator | Rubio López, Mónica | |
dc.creator | Morino, J. I. | |
dc.creator | Bronfman Aguiló, Leonardo | |
dc.creator | Handa, T. | |
dc.creator | Hatashi, M. | |
dc.creator | Nyman, L. A. | |
dc.creator | Oka, T. | |
dc.creator | Sakamoto, S. | |
dc.creator | Seta, M. | |
dc.creator | Usuda, K. S. | |
dc.date.accessioned | 2014-01-13T14:57:05Z | |
dc.date.available | 2014-01-13T14:57:05Z | |
dc.date.created | 2014-01-13T14:57:05Z | |
dc.date.issued | 2001-04-20 | |
dc.identifier | The Astrophysical Journal, 551:794-802, 2001 April 20 | |
dc.identifier | https://repositorio.uchile.cl/handle/2250/126210 | |
dc.description.abstract | We observed 34 positions throughout the disk of the Large Magellanic Cloud in the CO J = 21 emission line with the Tokyo-Onsala-ESO-Calán 60 cm radio telescope. Comparing the spectra with those of the J = 10 line at the same angular resolution (9, or 130 pc at 50 kpc), we found that the CO J = 21/J = 10 intensity ratio (R21/10) scatters in a range of 0.51.3. The luminosity ratio averaged for all observed points is 0.92 ± 0.05. The ratio R21/10 is approximately unity (0.95 ± 0.06) in 30 Dor, consistent with optically thick and thermalized emission, even in the southern part where massive star formation does not occur yet. This suggests that the high R21/10 is not primarily due to the UV radiation from young stars but rather to the intrinsic nature of the molecular gas that is relatively dense (103 cm-3) and may be ready to form stars. In addition to a cloud-to-cloud difference of R21/10, there exists a radial gradient of the ratio of 0.94 ± 0.11 in the inner region (2 kpc from the kinematic center) and 0.69 ± 0.11 in the outer region (2 kpc from the center, excluding the 30 Doradus complex). The higher R21/10 in the inner galaxy might be due to relatively higher gas densities within CO clumps in molecular clouds and/or higher external heating in that region. | |
dc.language | en_US | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Chile | |
dc.subject | galaxies : irregular | |
dc.title | The CO J = 21 / J = 10 Ratio in the Large Magellanic Cloud | |
dc.type | Artículo de revista | |