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pro vyhledávání: '"Levenson, LR"'
Autor:
Eales, SA, Smith, MWL, Wilson, CD, Bendo, GJ, Cortese, L, Pohlen, M, Boselli, A, Gomez, HL, Auld, R, Baes, Maarten, Barlow, MJ, Bock, JJ, Bradford, M, Buat, V, Castro-Rodriguez, N, Chanial, P, Charlot, S, Ciesla, L, Clements, DL, Cooray, A, Cormier, D, Davies, JI, Dwek, E, Elbaz, D, Galametz, M, Galliano, F, Gear, WK, Glenn, J, Griffin, M, Hony, S, Isaak, KG, Levenson, LR, Lu, N, Madden, S, O'Halloran, B, Okumura, K, Oliver, S, Page, MJ, Panuzzo, P, Papageorgiou, A, Parkin, TJ, Perez-Fournon, I, Rangwala, N, Rigby, EE, Roussel, H, Rykala, A, Sacchi, N, Sauvage, M, Schulz, B, Schirm, MRP, Spinoglio, L, Srinivasan, S, Stevens, JA, Symeonidis, M, Trichas, M, Vaccari, M, Vigroux, L, Wozniak, H, Wright, GS, Zeilinger, WW
Publikováno v:
ASTRONOMY & ASTROPHYSICS
The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______330::4ed9b8f74f6dd51b57a18803eeb86948
https://hdl.handle.net/1854/LU-1237016
https://hdl.handle.net/1854/LU-1237016
