Science with the Atacama Large Millimeter Array : A New Era for Astrophysics

Currently under construction in the Andean Altiplano, Northern Chile, the Atacama Large Millimeter Array (ALMA) is the most ambitious astronomy facility under construction. ALMA is a radio interferometer composed of 54 antennas of 12 m diameter, and twelve 7 m antennas with about 6600 square meters...

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সংরক্ষণ করুন:
গ্রন্থ-পঞ্জীর বিবরন
অন্যান্য লেখক: Bachiller, Rafael, 19..-...., astronome (Publishing director), Cernicharo, José, 1956- (Publishing director)
বিন্যাস: Livre numérique
ভাষা:Anglais
প্রকাশিত: Dordrecht : Springer Netherlands [20..].
Cham : Springer Nature
সংস্করন:1st ed. 2008.
অনলাইন ব্যবহার করুন:Accès sur la plateforme de l'éditeur
Accès sur la plateforme Istex
Accès Université d'Orléans
Accès INSA CVL
টীকা: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Variante du titre:Proceedings of the Conference held in Madrid (Spain), 13 17 November 2006
Edition sous un autre format:• Science with the Atacama Large Millimeter Array, a new era for astrophysics, proceedings of the Conference held in Madrid (Spain), 13-17 november 2006, Rafael Bachiller, José Cernicharo editors, 2008, New York, Springer, 1 vol. (335 p.), 1-402-06934-0
সূচিপত্রের সারণি:
  • The Atacama Large Millimeter/Submillimeter Array: overview & status ALMA capabilities for observations of spectral line emission ALMA capabilities for observations of continuum emission Star and planet-formation with ALMA: an overview High-mass star forming regions: An ALMA view Early stages of star formation Chemistry in low-mass star forming regions Molecular outflows observed with ALMA Unveiling the chemistry of hot protostellar cores with ALMA High resolution submillimeter observations of massive protostars High-resolution mm interferometry and the search for massive protostellar disks: the case of Cep-A HW2 The Class 0 source Barnard 1c APEX and ATCA observations of the southern hot core G327.3-0.6 and its environs The physical conditions in the BHR71 outflows Interstellar deuteroammonia Massive star formation in the southern Milky Way SMA observations of the magnetic fields around a low-mass protostellar system ASTE observations of the massive-star forming region Sgr B2: a giant impact scenario A new view of proto-planetary disks with ALMA Observational signature of planet formation: The ALMA view Detecting protoplanets with ALMA The study of young substellar objects with ALMA A submillimeter view of protoplanetary dust disks Studies of dense cores with ALMA Chemistry in the ISM: the ALMA (r)evolution High angular resolution imaging of the circumstellar material around intermediate mass (IM) stars Polarization measurements of molecular lines Molecular clouds and star formation in the Magellanic Clouds and the Milky Way Complex organic molecules in an early stage of protostellar evolution Revealing the fingerprints of the magnetic precursor of C-shocks A new evolutionary scenario of intermediate-mass star-formation revealed by multi-wavelength observations of OMC-2/3 Scientific role of ACA for low-mass star-formation study Planetary atmospheres with ALMA Cometary science with ALMA Observations of asteroids with ALMA ALMA as the ideal probe of the solar chromosphere The study of evolved stars with ALMA Molecular lines from protoplanetary nebulae: observations with ALMA Planetary nebulae and ALMA Chemistry in the circumstellar medium Understanding the chemical complexity in Circumstellar Envelopes of C-Rich AGB stars: the case of IRC +10216 New Plateau de Bure observations of M?1 92; unveiling the core A massive, dusty toroid with large grains in the pre-planetary nebula IRAS22036+5306 Gas dynamics and structure of galaxies Investigations of star formation in galaxies using ALMA Probing the feeding and feedback of activity near and far Chemical complexity in galaxies Chemistry in luminous AGN and starburst galaxies Dense gas in normal and active galaxies Spectroscopic surveys of cosmic evolution Observations of molecular clouds in nearby galaxies with ALMA