The distances to molecular clouds in the fourth Galactic quadrant

Abstract

Distance measurements to molecular clouds are essential and important. We present directly measured distances to 169 molecular clouds in the fourth quadrant of the Milky Way. Based on the near-infrared photometry from the Two Micron All Sky Survey and the Vista Variables in the Via Lactea Survey, we select red clump stars in the overlapping directions of the individual molecular clouds and infer the bin averaged extinction values and distances to these stars. We track the extinction versus distance profiles of the sightlines toward the clouds and fit them with Gaussian dust distribution models to find the distances to the clouds. We have obtained distances to 169 molecular clouds selected from Rice et al. The clouds range in distances between 2 and 11 kpc from the Sun. The typical internal uncertainties in the distances are less than 5 per cent and the systematic uncertainty is about 7 per cent. The catalogue presented in this work is one of the largest homogeneous catalogues of distant molecular clouds with the direct measurement of distances. Based on the catalogue, we have tested different spiral arm models from the literature.

9 pages, 7 figures, accepted for publication in MNRAS

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Cited by in corpus (4)

• Distances to molecular clouds in the second Galactic quadrant
• The diffuse interstellar band around 8620 Å I. Methods and application to the GIBS data set
• A large catalogue of molecular clouds in the southern sky
• The distances of 61 PGCCs in the Second Galactic Quadrant