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Vincent Toporenko
PIX4589595
Vincent Toporenko
PIX4589595
DGA507380
![Nebula LDN 988 in the Swan - LDN 988 nebula in Cygnus - Region around the dark nebula LDN 988 in the Swan. Area around the dark nebula LDN 988 with two blue reflection nebulae GN 21.01.3 and LBN 409. The emission nebula in the upper right of the image near the open cluster NGC 7031 seems uncataloged. Another interesting object is [C86] L988a. This is a looped nebula in LDN988. Sh2 - 120 and 121 are the two small HII regions left of center. Faint dust makes some of the background appear blue from reflection](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.98742640.7055475/4621610.jpg?old-wm)
![Clusters of distant galaxies RDCS1252.9 - 2927 - Distant galaxy cluster RDCS1252.9 - 2927 - This cluster of galaxies is 9 billion years old - light in the constellation Hydra, and is the most massive known to date. It probably contains several thousand galaxies. Image obtained by the Hubble Space Telescope and the VLT. The image shows the entire galaxy cluster (1/15 of a degree, corresponding to about 7 million light - years, across). The cluster probably contains many thousands of galaxies. Most of the other galaxies in the image, including most of the blue galaxies, are foreground or background galaxies. The image, which is made with an additional infrared exposure taken with the European Southern Observatory's Very Large Telescope, shows mature galaxies in a massive cluster that existed when the cosmos was 5000 million years old. The cluster, called RDCS1252.9 - 2927, is as massive as '300 trillion' suns and is the most massive known cluster for its epoch. Dominating the core are a pair of large, reddish elliptical galaxies [near centre of image]. Their red colour indicates an older population of stars. Most of the stars are at least 1000 million years old. The two galaxies appear to be interacting and may eventually merge to form a larger galaxy that is comparable to the brightest galaxies seen in present - day clusters. The red galaxies surrounding the central pair are also cluster members. The colour - composite image was assembled from two observations taken between May and June 2002 by the ACS Wide Field Camera, and one image with the ISAAC instrument on the VLT taken in 2002](https://images-cdn.bridgemanimages.com/api/1.0/image/600wm.PIX.75786540.7055475/4565578.jpg?old-wm)
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