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WFC3 SPECTROSCOPY OF THE MOST MASSIVE GALAXY PROTOCLUSTERS AT COSMIC NOON

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(AGENPARL) – LOW EARTH ORBIT, dom 15 novembre 2020 WFC3 Spectroscopy of the Most Massive Galaxy Protoclusters at Cosmic NoonHST Proposal 16276 Xin Wang (publications @ ADS)California Institute of Technology Cycle: 28Category: GalaxiesProposal type: GOStatus: implementation HST Proposal Information: about this proposal about other proposals by this PI Proposal Abstract......
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GOODS-ALMA: OPTICALLY DARK ALMA GALAXIES SHED LIGHT ON A CLUSTER IN FORMATION AT Z = 3.5

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(AGENPARL) – GARCHING (GERMANY), mer 11 novembre 2020 First Author: Zhou, L.Instruments: ALMA_Band_4, ALMA_Band_6, ALMA_Bands, HAWKI, ISAAC, VIMOSProgramIDs: 194.A-2003, 2015.1.00543.S, 2018.1.01079.S, 168.A-0485, 171.A-3045, 64.O-0643, 66.A-0572, 68.A-0544, 186.A-0898, 181.A-0717, 60.A-9284BibCode: 2020A&A…642A.155Z Thanks to its outstanding angular resolution, the Atacama Large Millimeter/submillimeter Array (ALMA) has recently unambiguously identified a population of optically......
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ALMA OBSERVATIONS OF NGC 6334S. I. FORMING MASSIVE STARS AND CLUSTERS IN SUBSONIC AND TRANSONIC FILAMENTARY CLOUDS

Redazione
(AGENPARL) – GARCHING (GERMANY), mer 11 novembre 2020 First Author: Li, ShanghuoInstruments: ALMA_Band_3, ALMA_Bands, LABOCAProgramIDs: 2016.1.00951.S, 181.C-0885, 078.F-9040, 079.C-9501, 081.C-9501, 080.F-9701, 082.F-9701, 085.F-9505, 085.F-9526BibCode: 2020ApJ…896..110L We present Atacama Large Millimeter/submillimeter Array (ALMA) and Karl G. Jansky Very Large Array (JVLA) observations of the massive infrared dark cloud NGC 6334S (also......
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MOST ISOLATED MASSIVE STARS ARE KICKED OUT OF THEIR CLUSTERS

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(AGENPARL) – ANN ARBOR (MICHIGAN), sab 31 ottobre 2020 A pair of University of Michigan studies reveals how some massive stars—stars eight or more times the mass of our sun—become isolated in the universe: most often, their star clusters kick them out. Massive stars typically reside in clusters. Isolated massive......
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STRUCTURAL EVOLUTION IN MASSIVE GALAXIES AT Z ∼ 2

Redazione
(AGENPARL) – GARCHING (GERMANY), dom 18 ottobre 2020 First Author: Tadaki, Ken-ichiInstruments: ALMA_Band_7, ALMA_BandsProgramIDs: 2012.1.00245.S, 2012.1.00983.S, 2013.1.00205.S, 2013.1.00566.S, 2013.1.00884.S, 2015.1.00242.S, 2016.1.01079.S, 2017.1.01027.SBibCode: 2020ApJ…901…74T We present 0″2 resolution Atacama Large Millimeter/submillimeter Array (ALMA) observations at 870 μm in a stellar mass-selected sample of 85 massive ( ${M}_{star }gt {10}^{11},{M}_{odot }$ <!–......
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SALT, HOT WATER, AND SILICON COMPOUNDS TRACING MASSIVE TWIN DISKS

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(AGENPARL) – GARCHING (GERMANY), mer 30 settembre 2020 First Author: Tanaka, Kei E. I.Instruments: ALMA_Band_3, ALMA_Band_6, ALMA_Band_7, ALMA_BandsProgramIDs: 2016.1.00992.S, 2018.1.01656.SBibCode: 2020ApJ…900L…2T We report results of $0buildrel{primeprime}over{.} 05$-resolution observations toward the O-type proto-binary system IRAS 16547-4247 with the Atacama Large Millimeter/submillimeter Array. We present dynamical and chemical structures of the circumbinary......
Agenparl English Ambiente Educazione Scienza e Tecnologia Social Network Video

ARE THE MOST MASSIVE STARS IN THE LOCAL GROUP TRULY SINGLE?

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(AGENPARL) – LOW EARTH ORBIT, lun 28 settembre 2020 Are the most massive stars in the Local Group truly single?HST Proposal 15942 Tomer Shenar (publications @ ADS)Katholieke Universiteit Leuven Cycle: 27Category: Stellar PhysicsProposal type: GOStatus: scheduling HST Proposal Information: about this proposal about other proposals by this PI Proposal Abstract......
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EMERGENCE OF AN ULTRARED, ULTRAMASSIVE GALAXY CLUSTER CORE AT Z = 4

Redazione
(AGENPARL) – GARCHING (GERMANY), ven 25 settembre 2020 First Author: Long, Arianna S.Instruments: ALMA_Band_3, ALMA_Band_4, ALMA_Band_7, ALMA_BandsProgramIDs: 2013.1.00001.S, 2013.1.00449.S, 2013.A.00014.S, 2016.1.01287.SBibCode: 2020ApJ…898..133L Recent simulations and observations of massive galaxy cluster evolution predict that the majority of stellar mass buildup happens within cluster members by z = 2, before cluster virialization.......

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