MALT90: The Millimetre Astronomy Legacy Team 90 GHz Survey
- Jackson, J. M.
- Rathborne, J. M.
- Foster, J. B.
- Whitaker, J. S.
- Sanhueza, P.
- Claysmith, C.
- Mascoop, J. L.
- Wienen, M.
- Breen, S. L.
- Herpin, F.
- Duarte-Cabral, A.
- Csengeri, T.
- Longmore, S. N.
- Contreras, Y.
- Indermuehle, B.
- Barnes, P. J.
- Walsh, A. J.
- Cunningham, M. R.
- Brooks, K. J.
- Britton, T. R.
- Voronkov, M. A.
- Urquhart, J. S.
- Alves, J.
- Jordan, C. H.
- Hill, T.
- Hoq, S.
- Finn, S. C.
- Bains, I.
- Bontemps, S.
- Bronfman, L.
- Caswell, J. L.
- Deharveng, L.
- Ellingsen, S. P.
- Fuller, G. A.
- Garay, G.
- Green, J. A.
- Hindson, L.
- Jones, P. A.
- Lenfestey, C.
- Lo, N.
- Lowe, V.
- Mardones, D.
- Menten, K. M.
- Minier, V.
- Morgan, L. K.
- Motte, F.
- Muller, E.
- Peretto, N.
- Purcell, C. R.
- Schilke, P.
- Bontemps, Schneider-N.
- Schuller, F.
- Titmarsh, A.
- Wyrowski, F.
- Zavagno, A.
DOIAbstract
The Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey aims to characterise the physical and chemical evolution of high-mass star-forming clumps. Exploiting the unique broad frequency range and on-the-fly mapping capabilities of the Australia Telescope National Facility Mopra 22msingle-dish telescope(1), MALT90 has obtained 3' x 3' maps towards similar to 2000 dense molecular clumps identified in the ATLASGAL 870 mu m Galactic plane survey. The clumps were selected to host the early stages of high-mass star formation and to span the complete range in their evolutionary states (from prestellar, to protostellar, and on to HII regions and photodissociation regions). Because MALT90 mapped 16 lines simultaneously with excellent spatial (38 ...
Add to ORKG