Zobrazeno 1 - 8
of 8
pro vyhledávání: '"H. Nieuwenhuyzen"'
Autor:
K. Murawski, N. Grevesse, S. Piteri, H. Nieuwenhuyzen, J. C. H. Van Der Hage, Vincent Icke, J. W. Hovenier, R. J. Rutten, J. P. De Greve, P. Kaufmann, G. Burki, Cornelis De Jager
Publikováno v:
Space Science Reviews. 65:365-372
Autor:
A. I. van de Vooren, H. Nieuwenhuyzen, B. N. Swanenburg, Josip Kleczek, B. R. A. Nyboer, D. W. Sciama, S. Mukai, H. Bokhove, W. I. Axford, G. Ooms, J. E. Guest, H. Wittenberg, A. G. G. M. Tielens
Publikováno v:
Space Science Reviews. 28:449-454
Autor:
J. L. Casse, J. van Amerongen, E. E. M. Woesterburg, J. Starre, Th. J. Helmerhorst, H. van de Stadt, J. van der Biezen, Th. de Graauw, H. Nieuwenhuyzen
Publikováno v:
SPIE Proceedings.
A submillimeter receiver, to be used as common-user receiver for UKIRT and the UK-NL mm telescope at Mau-na Kea, Hawaii, is here described. The receiver operates at two submm frequency bands using one backward wave oscillator (carcinotron) and a doub
Autor:
T. de Graauw, S. Lidholm, B. Fitton, F. P. Israel, A. Sargent, T. B. H. Kuiper, H. Nieuwenhuyzen
Publikováno v:
Interstellar Molecules ISBN: 9789400990999
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e0ee4435a77dde04765189f42edc9183
https://doi.org/10.1007/978-94-009-9097-5_29
https://doi.org/10.1007/978-94-009-9097-5_29
Publikováno v:
Interstellar Molecules ISBN: 9789400990999
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::98ffba72b0e5af3c9857d678e25b0ede
https://doi.org/10.1007/978-94-009-9097-5_32
https://doi.org/10.1007/978-94-009-9097-5_32
Autor:
T. de Graauw, S. Lidholm, B. Fitton, T.B.H. Kuiper, Frank P. Israel, H. Nieuwenhuyzen, A. I. Sargent
Publikováno v:
Symposium - International Astronomical Union. 87:115-116
We used the new OVRO 10 meter millimeter telescope together with the Estec heterodyne receiver and backend to observe 12CO (J=2-1) emission in the direction of several galactic HII regions. At a frequency of 230 GHz our angular resolution was 30 arcs
Autor:
B. Fitton, S. Lidholm, H. Nieuwenhuyzen, J. Vermue, Frank P. Israel, T. de Graauw, J. Beckman
Publikováno v:
Symposium - International Astronomical Union. 87:125-126
We used the ESO 3.6 m telescope at La Silla (Chile) in conjunction with the Estec heterodyne receiver to observe CO (J=2-1) emission from southern sources. The telescope HPBW was 2.2 arcmin, the beam efficiency 43 per cent. The receiver used backward
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