12CO and 13CO J=3-2 observations toward N11 in the Large Magellanic Cloud
arXiv:1905.08829 · doi:10.1051/0004-6361/201935446
Abstract
After 30 Doradus, N11 is the second largest and brightest nebula in the LMC. This large nebula has several OB associations with bright nebulae at its surroundings. N11 was previously mapped at the lowest rotational transitions of CO (J=1--0 and 2--1), and in some particular regions pointings of the CO J=1--0 and 2--1 lines were also performed. Using ASTE we mapped the whole extension of the N11 nebula in the CO J=3--2 line, and three sub-regions in the CO J=3--2 line. The regions mapped in the CO J=3--2 were selected based on that they may be exposed to the radiation at different ways: a region lying over the nebula related to the OB association LH10 (N11B), another one that it is associated with the southern part of the nebula related to the OB association LH13 (N11D), and finally a farther area at the southwest without any embedded OB association (N11I). We found that the morphology of the molecular clouds lying in each region shows some signatures that could be explained by the expansion of the nebulae and the action of the radiation. Fragmentation generated in a molecular shell due to the expansion of the N11 nebula is suggested. The integrated line ratios CO/CO show evidences of selective photodissociation of the CO, and probably other mechanisms such as chemical fractionation. The CO contribution to the continuum at 870 m was directly derived. The distribution of the integrated line ratios CO J=3--2/2--1 show hints of stellar feedback in N11B and N11D. The ratio between the virial and LTE mass (M/M) is higher than unity in all analyzed molecular clumps, which suggests that the clumps are not gravitationally bounded and may be supported by external pressure. A non-LTE analysis suggests that we are mapping gas with densities about a few 10 cm.
arXiv commentAccepted to be published in A&A. Figures were degraded
References in corpus (26)
- A computer program for fast non-LTE analysis of interstellar line spectra
- The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks
- The Second Survey of the Molecular Clouds in the Large Magellanic Cloud by NANTEN. II. Star Formation
- Bump Cepheids in the Magellanic Clouds: Metallicities, the Distances to the LMC and SMC, and the Pulsation-Evolution Mass Discrepancy
- Triggered massive-star formation on the borders of Galactic HII regions. I. A search for `collect and collapse' candidates
- The VLT-FLAMES survey of massive stars: Wind properties and evolution of hot massive stars in the LMC
- Star formation around RCW 120, the perfect bubble
- On-The-Fly Observing System of the Nobeyama 45-m and ASTE 10-m Telescopes
- Triggered star formation on the borders of the Galactic HII region RCW 82
- Star formation triggered by HII regions in our Galaxy: First results for N49 from the Herschel infrared survey of the Galactic plane
- Abundances and Isotope Ratios in the Magellanic Clouds: The Star Forming Environment of N113
- The CO/CO ratio in turbulent molecular clouds
- The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds
- Sub-millimeter Observations of Giant Molecular Clouds in the Large Magellanic Cloud: Temperature and Density as Determined from J=3-2 and J=1-0 transitions of CO
- Photodissociation regions and star formation in the Carina Nebula
- Further Evidence for Chemical Fractionation from Ultraviolet Observations of Carbon Monoxide
- C+ Emission from the Magellanic Clouds II. [CII] maps of star-forming regions LMC-N 11, SMC-N 66, and several others
- Active star formation in N11B Nebula in the Large Magellanic Cloud: a sequential star formation scenario confirmed
- Results of the ESO-SEST Key Programme on CO in the Magellanic Clouds. IX. The giant LMC HII region complex N11
- A view of Large Magellanic Cloud HII regions N159, N132, and N166 through the 345 GHz window
- ASTE observations in the 345 GHz window towards the HII region N113 of the Large Magellanic Cloud
- Detailed CO ( = 1--0, 2--1 and 3--2) observations toward an H{\sc ii} region RCW~32 in the Vela Molecular Ridge
- Triggered massive star formation associated with the bubble HII region Sh2-39 (N5)
- The dust properties and physical conditions of the interstellar medium in the LMC massive star forming complex N11
- Millimeter dust emission compared with other mass estimates in N11 molecular clouds in the LMC
- High Excitation Molecular Gas in the Galactic Center Loops; 12CO(J =2-1 and J =3-2) Observations
Cited by in corpus (5)
- ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
- Using CO line ratios to trace compressed areas in bubble N131
- SuperCAM CO(3-2) APEX survey at 6 pc resolution in the Small Magellanic Clouds
- Dense clumps survive in the vicinity of R136 in 30 Doradus
- Three-dimensional geometry and dust/gas ratios in massive star forming regions over the entire LMC as revealed by IRSF/SIRIUS survey