Robert Vudro Vilson — разлика између измена

 
Dok su radili na novom [[Holmdel Horn Antenna|tipu antena]] u [[Белове лабораторије|Belovim laboratorijama]] u [[Њу Џерзи|Nju Džerziju]],<ref name="nrhpinv">{{cite web | url={{NHLS url|id=89002457}} | last=Butowsky | first=Harry | title=Holmdel Horn Antenna | work=National Register of Historic Places Inventory-Nomination | publisher=[[National Park Service]] | date=1989-05-01}}</ref><ref>[http://www.nps.gov/history/nhl/designations/Lists/NJ01.pdf NJ NHL list]</ref><ref name="nhlsum">{{cite web|url=http://tps.cr.nps.gov/nhl/detail.cfm?ResourceId=2082&ResourceType=Structure|title=Holmdel Horn Antenna|date=2008-06-23|work=National Historic Landmark summary listing|publisher=National Park Service|url-status=dead|archiveurl=https://web.archive.org/web/20090225013531/http://tps.cr.nps.gov/nhl/detail.cfm?ResourceId=2082&ResourceType=Structure|archivedate=2009-02-25}}</ref> pronašli su šum koji nisu mogli da objasne.<ref>{{cite journal|last1=Penzias|first1 = A.A.|last2 = Wilson|first2=R.W.|title=A Measurement of Excess Antenna Temperature at 4080 Mc/s|journal=[[Astrophysical Journal]]|volume=142|pages=419–421|date=1965|doi=10.1086/148307|bibcode=1965ApJ...142..419P}}</ref><ref name="Penzias">{{cite journal | last1 = Penzias | first1 = A. A. | last2 = Wilson | first2 = R. W. | title = A Measurement of Excess Antenna Temperature at 4080 Mc/s | journal = Astrophysical Journal | volume = 142 | issue = | pages = 419–421 | publisher = [[American Astronomical Society]] | date = July 1965 | issn = | doi = 10.1086/148307 | id = | bibcode = 1965ApJ...142..419P}}</ref> Kada su odstranili sve potencijalne izvore, uključujući sletanje goluba na antenu, šum je konačno identifikovan kao [[Kosmičko pozadinsko zračenje|CMB]], koji je služio kao važna potvrda teorije [[Veliki prasak|Velikog praska]].
 
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InGodine 1970, WilsonVilson ledje apredvodio teamtim thatkoji madeje theostvario firstprvu detectiondetekciju ofrotacione aspektralne rotationallinije spectral line of carbon monoxideugljen monoksida (CO) in anu astronomicalastronomskom objectobjektu, the [[Orion Nebula|Orionovoj magli]], andi eightosam otherdrugih galacticgalaktičkih sourcesizvora.<ref>{{cite journal|last1=Wilson|first1 = R.W.|last2 = Jefferts|first2=K.B.|last3=Penzias|first3=A.A.|title=Carbon Monoxide in the Orion Nebula|journal=[[Astrophysical Journal]]|volume=161|pages=L43–L44|date=1970|doi=10.1086/180567|bibcode=1970ApJ...161..L43P}}</ref> SubsequentlyNakon toga, [[Carbon_monoxide#Astronomy|posmatranja CO observations]] becamesu thepostala standardstandardni methodmetod ofpraćenja tracinghladnog coolmolekularnog molecularmeđuzvezdanog interstellar gasgasa,<ref>{{cite journal|author=Combes, Françoise|year=1991|title=Distribution of CO in the Milky Way|journal=Annual Review of Astronomy & Astrophysics|volume=29|pages=195–237|bibcode=1991ARA&A..29..195C|doi=10.1146/annurev.aa.29.090191.001211}}</ref><ref>{{cite journal|author=Hamed, M.|year=2021|title=Multiwavelength dissection of a massive heavily dust-obscured galaxy and its blue companion at z∼2|journal=Astronomy & Astrophysics|volume=646|pages=A127|bibcode=2021A&A...646A.127H|doi=10.1051/0004-6361/202039577|arxiv=2101.07724|s2cid=231639096}}</ref><ref name="LAT-20140308">{{cite news|last=Khan|first=Amina|title=Did two planets around nearby star collide? Toxic gas holds hints|work=[[Los Angeles Times]]|url=http://www.latimes.com/science/sciencenow/la-sci-sn-beta-pictoris-star-planet-gas-collision-comets-carbon-monoxide-20140307,0,1884709.story|access-date=March 9, 2014}}</ref><ref name="SCI-20140306">{{cite journal|vauthors=Dent, WR, Wyatt, MC, Roberge, A, Augereau, JC, Casassus, S, Corder, S, Greaves, JS, ((de Gregorio-Monsalvo, I)), Hales, A, Jackson, AP, Hughes, AM, Meredith A, Lagrange, AM, Matthews, B, Wilner, D|date=March 6, 2014|title=Molecular Gas Clumps from the Destruction of Icy Bodies in the β Pictoris Debris Disk|url=https://www.science.org/doi/abs/10.1126/science.1248726|journal=[[Science (journal)|Science]]|volume=343|issue=6178|pages=1490–1492|arxiv=1404.1380|bibcode=2014Sci...343.1490D |doi=10.1126/science.1248726|pmid=24603151|access-date=March 9, 2014|s2cid=206553853}}</ref> anda detection ofdetekcija CO wasje thebila foundationaltemeljni eventdogađaj forza thepolja fieldsmilimetarske of millimeter andi [[Submillimetre astronomy|submillimetersubmilimetarske astronomyastronomije]].<ref name=ellesmere>{{cite web | url=http://almatelescope.ca/submmFuture-17feb2012/Presentations/Steinbring-Arctic.pdf | title=Recent Interest in Eureka on Ellesmere Island as a Submillimetre Observing Site | url-status=dead | archive-url=https://web.archive.org/web/20150703235656/http://almatelescope.ca/submmFuture-17feb2012/Presentations/Steinbring-Arctic.pdf | archive-date=2015-07-03 }}</ref><ref name=summit>{{cite web | url=http://www.asiaa.sinica.edu.tw/~hirashita/dust_group/JuanCarlos220811.pdf | title=ASIAA sub-mm VLBI Project}}</ref>
 
== Život i rad ==