RSGC1


RSGC1 is a young massive open cluster belonging to the Milky Way galaxy. It was discovered in 2006 in the data generated by several infrared surveys, named for the unprecedented number of red supergiant members. The cluster is located in the constellation Scutum at the distance of about 6.6 kpc from the Sun. It is likely situated at the intersection of the northern end of the Long Bar of the Milky Way and the inner portion of the Scutum–Centaurus Arm—one of its two major spiral arms.
The age of RSGC1 is estimated at 10–14 million years. The cluster is heavily obscured and has not been detected in the visible light. It lies close to other groupings of red supergiants known as Stephenson 2, RSGC3, Alicante 7, Alicante 8, and Alicante 10. The mass of RSGC1 is estimated at 30 thousand solar masses, which makes it one of the most massive open clusters in the Galaxy.
The observed red supergiants with the mass of about 16–20 solar masses are type II supernova progenitors. Over 200 main sequence stars have been detected with masses over, which allows the distance to be determined from main sequence fitting. Fourteen red supergiant members have been identified.
StarSpectral typeMagnitude Temperature Absolute magnitudeLuminosity Radius
F01M54.9623,300-3,450−11.75257,000-263,0001,435-1,551
F02M25.0293,600-3,660−11.92363,0001,498-1,549
F03M55.3333,200-3,450−11.28166,000-174,0001,168-1,326
F04M15.3423,752-3,900−11.24174,000-209,000914-1,082
F05M45.5353,535-3,600−11.36166,000-195,0001,047-1,177
F06M55.6133,300-3,450−10.70100,000885-967
F07M35.6313,600-3,605−10.8178,000-126,000718-910
F08M35.6543,605-3,700−11.33200,0001,088-1,146
F09M65.6703,100-3,399−10.92117,000-126,000986-1,231
F10M35.7093,500-3,605−10.86123,000-132,000931-954
F11M55.7223,535-3,600−11.03138,000-145,000955-1,015
F12M05.8643,200−10.7095,000-200,0001,003
F13K25.9574,015-4,100−11.39251,000-282,000993-1,098
F14M36.1673,500-3,605−10.2547,000-74,000590-697
F15G06.6826,850−10.07229,000340