คำอธิบายAntennae Galaxies composite of ALMA and Hubble observations.jpg
English: The Antennae Galaxies (also known as NGC 4038 and 4039) are a pair of distorted colliding spiral galaxies about 70 million light-years away, in the constellation of Corvus (The Crow). This view combines ALMA observations, made in two different wavelength ranges during the observatory’s early testing phase, with visible-light observations from the NASA/ESA Hubble Space Telescope.
The Hubble image is the sharpest view of this object ever taken and serves as the ultimate benchmark in terms of resolution. ALMA observes at much longer wavelengths which makes it much harder to obtain comparably sharp images. However, when the full ALMA array is completed its vision will be up to ten times sharper than Hubble.
Most of the ALMA test observations used to create this image were made using only twelve antennas working together — far fewer than will be used for the first science observations — and much closer together as well. Both of these factors make the new image just a taste of what is to come. As the observatory grows, the sharpness, speed, and quality of its observations will increase dramatically as more antennas become available and the array grows in size. This is nevertheless the best submillimetre-wavelength image ever taken of the Antennae Galaxies and opens a new window on the submillimetre Universe.
While visible light — shown here mainly in blue — reveals the newborn stars in the galaxies, ALMA’s view shows us something that cannot be seen at those wavelengths: the clouds of dense cold gas from which new stars form. The ALMA observations — shown here in red, pink and yellow — were made at specific wavelengths of millimetre and submillimetre light (ALMA bands 3 and 7), tuned to detect carbon monoxide molecules in the otherwise invisible hydrogen clouds, where new stars are forming.
Massive concentrations of gas are found not only in the hearts of the two galaxies but also in the chaotic region where they are colliding. Here, the total amount of gas is billions of times the mass of the Sun — a rich reservoir of material for future generations of stars. Observations like these will be vital in helping us understand how galaxy collisions can trigger the birth of new stars. This is just one example of how ALMA reveals parts of the Universe that cannot be seen with visible-light and infrared telescopes.
ALMA (ESO/NAOJ/NRAO). Visible light image: the NASA/ESA Hubble Space Telescope
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The Antennae Galaxies (also known as NGC 4038 and 4039) are a pair of distorted colliding spiral galaxies about 70 million light-years away, in the constellation of Corvus (The Crow). This view combines ALMA observations, made in two different wavelength ranges during the observatory’s early testing phase, with visible-light observations from the NASA/ESA Hubble Space Telescope. The Hubble image is the sharpest view of this object ever taken and serves as the ultimate benchmark in terms of resolution. ALMA observes at much longer wavelengths which makes it much harder toobtain comparably sharp images. However, when the full ALMA array is completed its vision will be up to ten times sharper than Hubble. Most of the ALMA test observations used to create this image were made using only twelve antennas working together — far fewer than will be used for the firstscience observations — and much closer together as well. Both of these factors make the new image just a taster of what is to come. As the observatory grows, the sharpness, speed, and quality of its observations will increase dramatically as more antennas become available and the array growsin size. This is nevertheless the best submillimetre-wavelength image ever taken of the Antennae Galaxies and opens a new window on the submillimetre Universe. While visible light — shown here mainly in blue — reveals the newborn stars in the galaxies, ALMA’s view shows us something that cannot be seen at those wavelengths: the clouds of dense cold gas from which new stars form. The ALMA observations — shown here in red, pink and yellow — were made at specific wavelengths of millimetre and submillimetre light (ALMA bands 3 and 7), tuned to detect carbon monoxide molecules inthe otherwise invisible hydrogen clouds, where new stars are forming. Massive concentrations of gas are found not only in the hearts of the two galaxies but also in the chaotic region where they are colliding. Here, the total amount of gas is billions of times the mass of the Sun — a rich reservoir of material for future generations of stars. Observations like these will be vital in helping us understand how galaxy collisions can trigger the birth of new stars. This is just one example of how ALMA reveals parts of the Universe that cannot be seen with visible-light and infrared telescopes. #L
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European Southern Observatory
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ALMA (ESO/NAOJ/NRAO). Visible light image: the NASA/ESA Hubble Space Telescope
ไฟล, antennae, galaxies, composite, alma, hubble, observations, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลาง, อม, ลเก, ยวก, บภาพขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, เมกะ. ifl prawtiifl hnathimiphaphni karichiflswnklang khxmulekiywkbphaphkhnadkhxngtwxyangni 602 600 phikesl khwamlaexiydxun 241 240 phikesl 482 480 phikesl 771 768 phikesl 1 028 1 024 phikesl 2 056 2 048 phikesl 3 375 3 362 phikesl duphaphthimikhwamlaexiydsungkwa 8206 3 375 3 362 phikesl khnadifl 2 95 emkaibt chnidimm image jpeg rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khwamyx khaxthibayAntennae Galaxies composite of ALMA and Hubble observations jpg English The Antennae Galaxies also known as NGC 4038 and 4039 are a pair of distorted colliding spiral galaxies about 70 million light years away in the constellation of Corvus The Crow This view combines ALMA observations made in two different wavelength ranges during the observatory s early testing phase with visible light observations from the NASA ESA Hubble Space Telescope The Hubble image is the sharpest view of this object ever taken and serves as the ultimate benchmark in terms of resolution ALMA observes at much longer wavelengths which makes it much harder to obtain comparably sharp images However when the full ALMA array is completed its vision will be up to ten times sharper than Hubble Most of the ALMA test observations used to create this image were made using only twelve antennas working together far fewer than will be used for the first science observations and much closer together as well Both of these factors make the new image just a taste of what is to come As the observatory grows the sharpness speed and quality of its observations will increase dramatically as more antennas become available and the array grows in size This is nevertheless the best submillimetre wavelength image ever taken of the Antennae Galaxies and opens a new window on the submillimetre Universe While visible light shown here mainly in blue reveals the newborn stars in the galaxies ALMA s view shows us something that cannot be seen at those wavelengths the clouds of dense cold gas from which new stars form The ALMA observations shown here in red pink and yellow were made at specific wavelengths of millimetre and submillimetre light ALMA bands 3 and 7 tuned to detect carbon monoxide molecules in the otherwise invisible hydrogen clouds where new stars are forming Massive concentrations of gas are found not only in the hearts of the two galaxies but also in the chaotic region where they are colliding Here the total amount of gas is billions of times the mass of the Sun a rich reservoir of material for future generations of stars Observations like these will be vital in helping us understand how galaxy collisions can trigger the birth of new stars This is just one example of how ALMA reveals parts of the Universe that cannot be seen with visible light and infrared telescopes wnthi 3 tulakhm ph s 2554 released aehlngthima http www eso org public images eso1137a phusrangsrrkh ALMA ESO NAOJ NRAO Visible light image the NASA ESA Hubble Space Telescope karxnuyatichsiththi This media was created by the European Southern Observatory ESO Their website states Unless specifically noted the images videos and music distributed on the public ESO website along with the texts of press releases announcements pictures of the week blog posts and captions are licensed under a Creative Commons Attribution 4 0 International License and may on a non exclusive basis be reproduced without fee provided the credit is clear and visible To the uploader You must provide a link URL to the original file and the authorship information if available iflnixyuphayitsyyaxnuyatkhriexthifkhxmmxns run aesdngthima 4 0 nanachatikhunsamarth thicaaebngpn thicathasaena aeckcay aelasngngandngklawtxip thicaeriyberiyngihm thicaddaeplngngandngklaw phayitenguxnikhtxipni aesdngthima khuntxngihekiyrtiecakhxngnganxyangehmaasm odyephimlingkipyngsyyaxnuyat aelarabuhakmikarepliynaeplng khunxacthaechnniidinrupaebbidkidtamkhwr aettxngimichinlksnathiaenawaphuihxnuyatsnbsnunkhunhruxkarichngankhxngkhunhttps creativecommons org licenses by 4 0 CC BY 4 0 Creative Commons Attribution 4 0 true truekhabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairxahrbالمجرات الهوائية التي تكونت من ملاحظات مرصد ألما وهابلixethmthiaesdngxyuiniflniprakxbdwysthanalikhsiththimilikhsiththisyyaxnuyatCreative Commons Attribution 4 0 International xngkvswnthisrang wnkxtng3 tulakhm 2011 prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn21 25 15 tulakhm 25553 375 3 362 2 95 emkaibt Stas1995 21 24 15 tulakhm 25552 048 1 536 1 07 emkaibt Stas1995 20 59 5 tulakhm 25543 375 3 362 2 96 emkaibt Jmencisom hnathimiphaphni hnatxipni oyngmathiphaphni darackrhnwdaemlng karichiflswnklang wikixuntxipniichiflni karichbn ar wikipedia org مصفوف مرصد أتاكاما المليمتري الكبير karichbn bn wikipedia org আত ক ম ল র জ ম ল ম ট র অ য র karichbn cs wikipedia org Tykadla galaxie Wikipedista Paul E NGC 501 karichbn de wikipedia org Atacama Large Millimeter submillimeter Array karichbn el wikipedia org Megalh Xiliostometrikh Diata3h ths Atakama karichbn en wikipedia org Atacama Large Millimeter Array Antennae Galaxies karichbn en wikiversity org Draft Original research Radiation astronomy User Marshallsumter Radiation astronomy2 Submillimeters User Marshallsumter Radiation astronomy Courses Principles Hourly 2 Draft Original research Chemicals User Marshallsumter Radiation astronomy1 Galaxies User Marshallsumter Radiation astronomy1 Molecules Portal Radiation astronomy Resource Portal Radiation astronomy Resource 30 Radiation Astronomy Chemicals Oxygens User Marshallsumter Radiation astronomy Chemicals karichbn fa wikipedia org دوشاخک karichbn fr wikipedia org Grand reseau d antennes millimetrique submillimetrique de l Atacama Galaxies des Antennes NGC 4039 karichbn ja wikipedia org アタカマ大型ミリ波サブミリ波干渉計 karichbn ka wikipedia org საცეცების გალაქტიკები karichbn lb wikipedia org Atacama Large Millimeter Array karichbn oc wikipedia org Atacama Large Millimeter Array karichbn ru wikipedia org Galaktiki Antenny karichbn sk wikipedia org Tykadla galaxie karichbn sr wikipedia org Atacama veliki milimetarski niz karichbn vi wikipedia org Thien ha Rau karichbn zh wikipedia org 阿塔卡馬大型毫米波 亞毫米波陣列khxmulekiywkbphaph phaphnimikhxmulephimetim sungswnihymacakklxngdicitxlhruxsaeknenxrthisamarthekbkhxmuldngklawiwrwmkbphaphid thaphaphnithukprbprungaekikhhruxepliynaeplngcakedim khxmulbangxyangcayngkhngimepliynaeplngehmuxnphaphthithukprbprungaekikhnnchuxphaphThe Antennae Galaxies also known as NGC 4038 and 4039 are a pair of distorted colliding spiral galaxies about 70 million light years away in the constellation of Corvus The Crow This view combines ALMA observations made in two different wavelength ranges during the observatory s early testing phase with visible light observations from the NASA ESA Hubble Space Telescope The Hubble image is the sharpest view of this object ever taken and serves as the ultimate benchmark in terms of resolution ALMA observes at much longer wavelengths which makes it much harder toobtain comparably sharp images However when the full ALMA array is completed its vision will be up to ten times sharper than Hubble Most of the ALMA test observations used to create this image were made using only twelve antennas working together far fewer than will be used for the firstscience observations and much closer together as well 160 Both of these factors make the new image just a taster of what is to come As the observatory grows the sharpness speed and quality of its observations will increase dramatically as more antennas become available and the array growsin size This is nevertheless the best submillimetre wavelength image ever taken of the Antennae Galaxies and opens a new window on the submillimetre Universe While visible light shown here mainly in blue reveals the newborn stars in the galaxies ALMA s view shows us something that cannot be seen at those wavelengths the clouds of dense cold gas from which new stars form The ALMA observations shown here in red pink and yellow were made at specific wavelengths of millimetre and submillimetre light ALMA bands 3 and 7 tuned to detect carbon monoxide molecules inthe otherwise invisible hydrogen clouds where new stars are forming Massive concentrations of gas are found not only in the hearts of the two galaxies but also in the chaotic region where they are colliding Here the total amount of gas is billions of times the mass of the Sun a rich reservoir of material for future generations of stars Observations like these will be vital in helping us understand how galaxy collisions can trigger the birth of new stars This is just one example of how ALMA reveals parts of the Universe that cannot be seen with visible light and infrared telescopes Lewlathibnthukphaph11 30 3 tulakhm 2554sthanalikhsiththiimidkahndsthanalikhsiththikhaklawlikhsiththixxnilntnchbbEuropean Southern Observatoryekhrdit phucdetriymALMA ESO NAOJ NRAO Visible light image the NASA ESA Hubble Space TelescopekhxtklnginkarichnganCreative Commons Attribution 3 0 Unported license chuxeruxngsnAntennae Galaxies composite of ALMA and Hubble observationskhasakhyAntennae Galaxies NGC 4038 NGC 4039khxmulsahrbtidtxhttp www eso org Karl Schwarzschild Strasse 2Garching bei Munchen D 85748 Germanykarihkhaaenn cak 5 5 ekhathungcak https th wikipedia org wiki ifl Antennae Galaxies composite of ALMA and Hubble observations jpg, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
