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The early observations of G237 implied it was creating stars at an unrealistically high and unsustainable rate. "Each of the 63 galaxies discovered so far in G237 was like a star factory in ...
G237 is so far away that its light traveled for more than 10.6 billion years. Several instruments joined forces to produce this image of the G237 protocluster, identifying its galaxies in different colors representing different wavelengths of observations. The image on the right zooms in on the central region of G237.
General Electric G237 - Does anyone know what year this was manufactured? This was my grandpa's. I believe it was built between 1967-1969 due to the enclosed speaker system but I can't find anything to pin down a more concrete date. Any help would be appreciated!
At first, observations of G237 implied a total star formation rate that was unrealistically high, and the team struggled to make sense of the data. The G237 protocluster seemed to be forming stars at a rate of 10,000 times that of the Milky Way. At that rate, the protocluster would be expected to rapidly use up its stellar fuel and subsequently ...
The Planck satellite has identified more than 2000 protocluster candidates with extreme star formation rates (SFRs). Here, we present the spectroscopic identification of a Planck-selected protocluster located in the Cosmos field, PHz G237.01+42.50. PHz G237.01+42.50 contains a galaxy overdensity of 31 spectroscopically identified galaxies at z ≃ 2.16 (significant at 5.4σ) in a 10′ × 11 ...
The Planck satellite has identified more than 2000 protocluster candidates with extreme star formation rates (SFRs). Here, we present the spectroscopic identification of a Planck-selected protocluster located in the Cosmos field, PHz G237.01+42.50 (G237). G237 contains a galaxy overdensity of 31 spectroscopically identified galaxies at z~2.16 (significant at 5.4 sigma) in a 10'x11' region. The ...
At a redshift of approximately 2.16, PHz G237.01+42.50 (or G237 for short) is a galaxy protocluster detected with the Planck satellite. The object was first reported in the Planck high-z (PHz ...
At first, observations of G237 implied a total star formation rate that was unrealistically high, and the team struggled to make sense of the data. The G237 protocluster seemed to be forming stars ...
PHz G237.01+42.50 contains a galaxy overdensity of 31 spectroscopically identified galaxies at z ≃ 2.16 (significant at 5.4σ) in a 10′ × 11′ region. The overdensity contains two substructures or protoclusters at z ≃ 2.16 and 2.195 with estimated halo masses at z = 0 of ∼5-6 × 10 14 M ⊙ , roughly consistent with Virgo-type clusters.
been obtained, PHzG237.01+42.50 (G237). The advantage of using this field is the availability of a wealth of multiwavelength data, in particular of spectroscopic redshifts, that allow us to identify and analyze the protocluster member galaxies. Throughout this work we use magnitudes in the AB sys-