Results 41 to 50 of about 739 (176)
SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data [PDF]
We measure the 850-μm source densities of 46 candidate protoclusters selected from the Planck High-z catalogue (PHz) and the Planck Catalogue of Compact Sources (PCCS) that were followed up with Herschel -SPIRE and SCUBA-2.
Ibar, Eduardo
core +4 more sources
The internal structure of protoclusters and the formation of galaxies [PDF]
We give a short review of the general picture and main features of the formation of galaxies and clusters of galaxies on the basis of the adiabatic theory. Detailed discussions of these questions are published in references 1–6. Some related problems of the formation and development of large scale structure in the Universe according to the same theory ...
A. G. Doroshkevich +2 more
openaire +1 more source
LCDM predictions for galaxy protoclusters I: the relation between galaxies, protoclusters and quasars at z~6 [PDF]
Accepted by MNRAS (19 pages, 20 figures, 2 tables).
Overzier, R. +5 more
openaire +5 more sources
DISCOVERY OF A PROTOCLUSTER ATz∼ 6 [PDF]
12 pages, 9 figures, accepted for publication in ...
Toshikawa, Jun +12 more
openaire +3 more sources
SPECTROSCOPIC CONFIRMATION OF A PROTOCLUSTER AT z ≈ 3.786 [PDF]
ABSTRACT We present new observations of the field containing the z = 3.786 protocluster PC 217.96+32.3. We confirm that it is one of the largest known and most overdense high-redshift structures. Such structures are rare even in the largest cosmological simulations. We used the Mayall/MOSAIC1.1 imaging camera to image a 1.°2 × 0.°6 area (
Arjun Dey +7 more
openaire +4 more sources
Understanding Starbursting Protoclusters: Follow-up of Herschel-Planck Selected Sources [PDF]
Crossmatching between Planck and Herschel data has uncovered a total of 30 high-z candidate starbursting protoclusters in HerMES & H-ATLAS. These protoclusters might be in their formation period so their study is important in characterising cluster ...
Cheng, Tai-An (5366761) +5 more
core +1 more source
Protoclusters in the ΛCDM Universe
We compare the highly clustered populations of very high redshift galaxies with protoclusters identified numerically in a standard ΛCDM universe (Ω0 = 0.3, λ0 = 0.7) simulation. We evolve 2563 dark matter particles in a comoving box of side 150 h-1 Mpc.
Tamon Suwa, Asao Habe, Kohji Yoshikawa
openaire +1 more source
FRAGMENTATION OF MOLECULAR CLUMPS AND FORMATION OF A PROTOCLUSTER [PDF]
Sufficiently massive clumps of molecular gas collapse under self-gravity and fragment to spawn a cluster of stars that have a range of masses. We investigate observationally the early stages of formation of a stellar cluster in a massive filamentary infrared dark cloud, G28.34+0.06 P1, in the 1.3mm continuum and spectral line emission using the ALMA ...
Qizhou Zhang +3 more
openaire +2 more sources
A giant protocluster of galaxies at redshift 5.7 [PDF]
Galaxy clusters trace the largest structures of the Universe and provide ideal laboratories for studying galaxy evolution and cosmology. Clusters with extended X-ray emission have been discovered at redshifts up to z ~ 2.5. Meanwhile, there has been growing interest in hunting for protoclusters, the progenitors of clusters, at higher redshifts.
Jiang, L. +15 more
openaire +4 more sources
Competitive accretion in the protocluster G10.6−0.4? [PDF]
9 pages, 9 figures, 2 tables, Submitted to ...
Liu, Tie +4 more
openaire +2 more sources

