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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...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor Corporativo: | |
| Otros Autores: | , |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Dordrecht :
Springer Netherlands : Imprint: Springer,
2008.
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| Edición: | 1st ed. 2008. |
| Temas: | |
| Acceso en línea: | Texto Completo |
Tabla de Contenidos:
- 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
- Luminous infrared galaxies with the submillimeter array: probing the extremes of star formation
- The Galactic Center as nearby extragalactic chemical laboratory
- Studying the first galaxies with ALMA
- Detecting the most distant (z>7) objects with ALMA
- Redshift distribution of the submillimeter extragalactic background light
- Molecular absorptions in high-z objects
- Molecular signature of star formation at high redshifts
- Dense molecular gas in a sample of LIRGs and ULIRGs: The low-redshift connection to the huge high-redshift starbursts and AGNs.