PDF-Nobeyama CO Atlas of Nearby Spiral Galaxies

Author : conchita-marotz | Published Date : 2015-09-11

Kuno N 1 Sato N 12 Nakanishi H 1 Hirota A 13 Tosaki T 1 Shioya Y Nakai N 5 Sorai K 2 Nishiyama K 6 Ishihara Y 7 VilaVilar

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Nobeyama CO Atlas of Nearby Spiral Galaxies: Transcript


Kuno N 1 Sato N 12 Nakanishi H 1 Hirota A 13 Tosaki T 1 Shioya Y Nakai N 5 Sorai K 2 Nishiyama K 6 Ishihara Y 7 VilaVilar. 16. The Tale of the Ale. 2. spiral. 16. Topic. Total Pages. Domains. Date. Range. Pages/Day. Boulevard Brewing Co.. 4148. 1077. 10/6/11. – 1/24/12. 46. Chocolate Ale. 1873. 280. 1/24/12 – 2/9/2012. Low-. Redshift. Galaxies. Adam Leroy (NRAO, North American ALMA Science Center). HERACLES & THINGS teams: . Fabian Walter, Andreas . Schruba. , Frank . Bigiel. , Elias Brinks, Erwin . de . Blok, Kelly . Except for nearby, we can only see bright galaxies. I will ignore dwarf . spheroidal. (. dSph. ) and dwarf elliptical (. dE. ) classifications. Galaxies . come in four broad categories, based on their appearance. Li Jiang-Tao. 1. Service d’Astrophysique, CEA, Saclay, France. 2. . Department. of . Astronomy. , . University. of Michigan, Ann Arbor, USA. Outline. 1. Introduction. 2. Diffuse X-ray . observation. D. Calzetti (Univ. of Massachusetts). a. nd the LEGUS . Team. https://. legus.stsci.edu. /. HUBBLE2020: Hubble’s 25. th. Anniversary Symposium. STScI. , Baltimore, April 20-24, 2015. NGC3344. NGC1566. 2. The Universe. Th. 3. The Universe is . everything. t. hat exists in space. 4. Galaxies. 5. Galaxies and Shapes (…Cont.). Spiral galaxies:. can be broken down in two categories. Circular spiral - round center. around Abell 370, . a galaxy cluster at z = 0.37. International SKA . Forum 2010 . Philip Lah. A New Golden Age for Radio Astronomy. Collaborators:. . Frank Briggs (ANU). . Michael Pracy . By. Chris . W. ilson. And. Geoff . Zelder. History. Pedro . Nunes. , a sixteenth century Portuguese cosmographer discovered that the shortest distance from point A to point B on a sphere is not a straight line, but an arc known as the great circle route.. megaparsecs. away be moving with respect to us, according to Hubble’s Law? Hint: H. 0. = 70 km/s/. Mpc. 1,400 km/s. 14,000 km/s. 140,000 km/s. 140 km/s. How fast would a galaxy 2,000 . megaparsecs. in the Universe?. What is the solar system?. The solar system consists of:. The sun (which is the name of our star). Planets . Asteroids . Comets . Space rocks . Measurement in Astronomy. Scientists find it hard to work with the measurements we use on earth, like kilometers and miles, because the distances are so great it is hard for us to comprehend such enormous numbers. . Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Chapter 2. Stars. Section 1 Vocabulary. Spectrum. Apparent Magnitude. Absolute Magnitude. Light-Year. Parallax. Color of Stars. Red and Yellow. Cool. Blue . Warm. Blue flame hotter than yellow flame. Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation.

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