Science Case
The ngVLA will have broad impact on many of the high priority goals of modern astronomy & astrophysics, including the science priorities described in the New Worlds, New Horizons Astro2010 Decadal Survey. The ngVLA Science Working Groups (SWGs) have identified a number of key science programs that push the requirements of the telescope through a community driven Science Use Case capture exercise that led by the ngVLA Science Advisory Council. Information on submitting additional ngVLA Science Use Cases, along with the list of current use cases, is given below.
If you are interested in joining one of the Science Working Groups, please contact the corresponding science working group chair directly. An initial set of science goals suggested by the four SWGs are described in white papers published in the ngVLA memo series.
ngVLA Science Use Cases -- Submission Material Here
A current list of all ngVLA Science Use Cases received is available. If you are interested in submitting a new ngVLA Science Use Case, please fill out the following form (ngVLA Science Use Cases Form) and submit it to the appropriate ngVLA Science Working Group chair. An example of a filled out Science Use Case form can be found here (example ngVLA Science Use Case Form). For full consideration, please submit your Science Use Case by December 2017.
ngVLA Key Science Drivers
As examples, three compelling science goals that require an ngVLA are briefly described below. The Science Working Groups are continuing to expand their science programs through realistic simulations, and a corresponding science workshop highlighting their findings will be held in 2017.
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Image the inner "terrestrial-zone" of planet formation in protoplanetary disksThe inner regions of protoplanetary disks are optically thick at shorter wavelengths. The ngVLA will image gap-structures indicating planet formation on solar system scales, determine the growth of grains, and image accretion onto porto-planets themselves. Probing dust gaps on 1 AU scales in the nearest major star-forming regions requires baselines 10x the Jansky VLA baselines, with a sensitivity adequate to achieve a few K brightness at 1 cm wavelength and 9 mas resolution.
Probe interstellar medium & star formation physics on scales from Giant Molecular Clouds down to cloud cores out to VirgoThe ngVLA covers the spectral range richest in the ground state transitions of the most important molecules in astrochemistry and astrobiology, as well as key thermal and non-thermal continuum emission processes related to star formation. The ngVLA will perform wide field imaging of line and continuum emission on scales from GMCs (100 pc) down to cores (few pc) in galaxies out to the Virgo Cluster, with an order of magnitude faster mapping speed than ALMA. A centrally condensed antenna distribution on scales of a few to 10 km is required for wide-field, high surface brightness sensitivity.
Census the cold molecular gas fueling star formation back to the first galaxiesOctave bandwidth is required for large cosmic volume surveys of low order CO emission (the fundamental tracer of total gas mass) from distant galaxies, as well as for dense gas tracers such as HCN and HCO+. The spatial resolution and sensitivity will also be adequate to image the gas on sub-kph scales and detect molecular gas masses down to dwarf galaxies. |
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