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2020ApJS..249...27L - Astrophys. J., Suppl. Ser., 249, 27-27 (2020/August-0)

The molecular clouds associated with the H II regions/candidates between L = 207°.7 and L = 211°.7.

LI C., WANG H., ZHANG M., MA Y. and LIN L.

Abstract (from CDS):

Using the PMO-13.7 m millimeter telescope at Delingha in China, we have conducted a large-scale simultaneous survey of 12CO, 13CO, and C18O J = 1 - 0 emission toward the sky region centered at l = 209.°7, b = -2.°25 with a coverage of 4.°0 x 4.°5. The majority of the emission in the region comes from the clouds with velocities lying in the range from -3 to 55 km s–1, at kinematic distances from 0.5 to 7.0 kpc. The molecular clouds in the region are concentrated into three velocity ranges. The molecular clouds associated with the 10 H II regions/candidates are identified and their physical properties are presented. Massive stars are found within Sh2-280, Sh2-282, Sh2-283, and BFS54, and we suggest them to be the candidate excitation sources of the H II regions. The distributions of the excitation temperature and line width with the projected distance from the center of H II region/candidate suggest that the majority of the 10 H II regions/candidates and their associated molecular gas are three-dimensional structures, rather than two-dimensional structures.

Abstract Copyright: © 2020. The American Astronomical Society. All rights reserved.

Journal keyword(s): H II regions - Molecular spectroscopy - Molecular clouds

Simbad objects: 28

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2021.12.07-10:26:57

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