1,720,979 research outputs found
Replication Data for: Distances of 28 local molecular clouds in the first Galactic quadrant
No full text28 molecular clouds in total
Distances to 76 local molecular clouds in the second Galactic quadrant
No full text76 molecular cloud
Replication Data for: Catalogs of molecular clouds in the first Galactic latitudes
No full textThe table is in FITS format, which can be read with Table package in astropy.
Naming convention:
DBSCAN
Replication Data for: Distances of 28 local molecular clouds in the first Galactic quadrant
No full text28 molecular clouds in total
The distance catalog and figures for "Improved Measurements of Molecular Cloud Distances Based on Global Search"
No full text145 distance cases and corresponding figure
The 13CO (J=1-0) velocity (VLSR) of HII region candidates (Table B.1)
No full textTable B.1 in the paper
Replication Data for: The distances to molecular clouds at high Galactic latitudes with Gaia DR2
No full textAll the molecular-cloud-distance figures calculated with the Markov chain Monte Carlo (MCMC) method
The 13CO (J=1-0) velocity (VLSR) of HII region candidates (Table B.1)
No full textTable B.1 in the paper
12 GHz methanol maser outflow from the massive star-forming region: G35.20-0.74
No full textWe report the internal proper motions of 12 GHz methanol masers in massive star-forming region G35.20-0.74 observed with the Very Long Baseline Array (VLBA) at four epochs spanning about 1.5 yr. Two groups of maser features were detected, groups A and B, and the latter that had a V-shaped spatial distribution is likely tracing the north outflow in G35.20-0.74. We present a three-dimensional model for the kinematics of these masers, by assuming the interstellar medium was blown by the stellar wind from the driving source (G35.2N) of the outflow. Adopting a position angle of similar to 81 degrees for the main axis of the outflow from previous studies, we estimate an inclination of 35 degrees +/- 5.5 degrees, a velocity of 8.1 +/- 0.7 km s(-1) for the stellar wind along the main axis and an expansion speed gradient of 0.05 +/- 0.016 km s(-1) AU(-1). From the model, we derive the age of the north outflow in G35.20-0.74 to be similar to 1.6 x 10(4) yr
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