List of star-forming regions in the Local Group explained

This is a list of star-forming regions located in the Milky Way Galaxy and in the Local Group. Star formation occurs in molecular clouds which become unstable to gravitational collapse, and these complexes may contain clusters of young stars and regions of ionized gas called H II regions. Stars typically form in groups of many stars, rather than in isolation.

Galactic star-forming regions

Name data-sort-type="number" RA [deg] data-sort-type="number" Dec [deg]data-sort-type="number" l [deg]data-sort-type="number" b [deg]data-sort-type="number" Distance [pc]data-sort-type="number" Age [Myr]Earliest SpTydata-sort-type="number" Number of Starsdata-sort-type="number" Cloud Mass [Mo]
287.368 -37.904 130
247.025 -24.541 353.22 16.53 131
070.25 +25.87174.13 -13.45 140
83.8221 -5.3911 209.013 -19.382 415
277.871 -2.090 28.791 +3.481 500 0.8 late-O 520
134.7537 -43.0 265.0794 +1.4048 700
134.7537 -43.0 265.0794 +1.4048 700-1000
307.5 41.0 1400
260.212 -36.115351.42+0.641700
261.62 -34.20 353.11+0.65 1700
274.700 -13.807 16.95 +0.793 1750
275.196 -16.172 15.06 -0.69 2000
161.285 -59.868 2600
307.354 40.189 078.887 +0.709 3300 O9–O6
281.885 -01.942 30.759 -0.019 6000
287.582 +9.128 43.200 +0.000 11000 O2-3.5If*
Radcliffe wave[1]

Extragalactic star-forming regions

Name data-sort-type="number" RA [deg] data-sort-type="number" Dec [deg]data-sort-type="number" l [deg]data-sort-type="number" b [deg]data-sort-type="number" Distance [pc]data-sort-type="number" Age [Myr]Earliest SpTydata-sort-type="number" Number of Starsdata-sort-type="number" Cloud Mass [Mo]
84.67665 -69.10093 279.4652 -31.6719 49,000

See also

References

  1. News: Ian. Sample. 2020-01-07. Astronomers discover huge gaseous wave holding Milky Way's newest stars. The Guardian. 7 January 2020. 0261-3077. www.theguardian.com.

[2] [3] [4] [5] [6] [7] [8] [9] [10]

External links