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  2. MACS J0717.5+3745 - Wikipedia

    en.wikipedia.org/wiki/MACS_J0717.5+3745

    The cluster was formed by four separate galaxy clusters that have been involved in a collision. This is the first time that this phenomenon has been observed. The repeated collisions in MACSJ0717 are caused by a 13-million-light-year-long stream of galaxies, gas, and dark matter, known as a filament, pouring into a region already full of matter ...

  3. MACS J0416.1-2403 - Wikipedia

    en.wikipedia.org/wiki/MACS_J0416.1-2403

    MACS J0416.1-2403 or MACS0416 abbreviated, is a cluster of galaxies at a redshift of z=0.397 with a mass 160 trillion times the mass of the Sun inside 200 kpc (650 kly).Its mass extends out to a radius of 950 kpc (3,100 kly) and was measured as 1.15 × 10 15 solar masses. [2]

  4. NGC 6939 - Wikipedia

    en.wikipedia.org/wiki/NGC_6939

    NGC 6939 is an old open cluster, located 400 parsec above the galactic plane and 8.400 parsec away from the galactic centre. [5] With the use of photometric studies, the age of the cluster was estimated to be between 1,0 and 1,3 billion years!, using as sample 638 stars within the field.

  5. IC 4756 - Wikipedia

    en.wikipedia.org/wiki/IC_4756

    There are some noteworthy stars in the cluster. HD 172365 [5] is a likely post-blue straggler in the IC 4756 that contains a large excess of lithium. [6] HD 172189, also in IC 4756, is an Algol variable eclipsing binary [7] with a 5.70 day period. The primary star in the system is also a Delta Scuti variable, undergoing multiple pulsation ...

  6. Messier 15 - Wikipedia

    en.wikipedia.org/wiki/Messier_15

    Messier 15 or M15 (also designated NGC 7078 and sometimes known as the Great Pegasus Cluster) is a globular cluster in the constellation Pegasus. It was discovered by Jean-Dominique Maraldi in 1746 and included in Charles Messier 's catalogue of comet -like objects in 1764.

  7. Abell 2744 - Wikipedia

    en.wikipedia.org/wiki/Abell_2744

    Abell 2744, nicknamed Pandora's Cluster, is a giant galaxy cluster resulting from the simultaneous pile-up of at least four separate, smaller galaxy clusters that took place over a span of 350 million years, and is located approximately 4 billion light years from Earth. [1] The galaxies in the cluster make up less than five percent of its mass. [1]