Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Tui Britton"'
Autor:
Paul Jones, Shari Breen, S. N. Longmore, James Urquhart, Matthew Whiting, N. Lo, Cormac Purcell, B. Indermuehle, Lisa Harvey-Smith, Maggie A. Thompson, Melvin Hoare, Tui Britton, Maxim Voronkov, Maria Cunningham, Graeme L. White, Luke Hindson, Chris Phillips, Vicki Lowe, Michael G. Burton, Andrew Walsh, K. J. Brooks, J. A. Green
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 426:1972-1991
The H2O Southern Galactic Plane Survey (HOPS) has mapped a 100 degree strip of the Galactic plane (-70deg > l > 30deg, |b| 10^4 cm^{-3}). In this paper we present the NH3 (1,1) and (2,2) data, which have a resolution of 2 arcmin and cover a velocity
Autor:
Andrew Walsh, Luke Hindson, K. J. Brooks, N. Lo, Shari Breen, Maria Cunningham, Michael G. Burton, J. A. Green, Melvin Hoare, Cormac Purcell, S. N. Longmore, Graeme L. White, Lisa Harvey-Smith, Chris Phillips, Vicki Lowe, B. Indermuehle, Tui Britton, Maxim Voronkov, Paul Jones, Maggie A. Thompson, Matthew Whiting, James Urquhart
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 416:1764-1821
We present first results of the H_2O Southern Galactic Plane Survey (HOPS), using the Mopra radiotelescope with a broad band backend and a beam size of about 2'. We have observed 100 square degrees of the southern Galactic plane at 12mm (19.5 to 27.5
Autor:
Kate J. Brooks, Cormac Purcell, Andrew Walsh, Tui Britton, Maxim Voronkov, Graeme L. White, Matthew Whiting, Vicki Lowe, B. Indermuehle, Paul A. Jones, James Green, Shari Breen, Chris Phillips, Michael G. Burton, N. Lo, Steven N. Longmore, James Urquhart, Michelle Thompson, Luke Hindson, Melvin Hoare, Maria Cunningham, Lisa Harvey-Smith
Publikováno v:
EAS Publications Series. 52:135-138
Over the past 3 years, we have conducted a survey of 100 square degrees of the southern Galactic plane with the Mopra radiotelescope (HOPS). The survey includes observations of multiple spectral lines in the 12 mm band, with the most important being
Autor:
Timea Csengeri, Jill Rathborne, Steven N. Longmore, Sadia Hoq, M. Wienen, Andrew Walsh, Fabrice Herpin, Tui Britton, Maxim Voronkov, Shari Breen, Jonathan B. Foster, Tracey Hill, Christopher H. Jordan, K. J. Brooks, Christopher Claysmith, Patricio Sanhueza, Joshua L. Mascoop, Ana Duarte-Cabral, Peter J. Barnes, Balthasar T. Indermuehle, Maria Cunningham, J. S. Whitaker, James Urquhart, Yanett Contreras, James M. Jackson, João Alves
Publikováno v:
Publications of the Astronomical Society of Australia
Publications of the Astronomical Society of Australia, Cambridge University Press (CUP), 2013, 30, pp.id.e038. ⟨10.1017/pasa.2013.18⟩
Publications of the Astronomical Society of Australia, Cambridge University Press (CUP), 2013, 30, pp.id.e038. ⟨10.1017/pasa.2013.18⟩
We characterize the Millimeter Astronomy Legacy Team 90 GHz (MALT90) Survey and the Mopra telescope at 90 GHz. We combine repeated position-switched observations of the source G300.968+01.145 with a map of the same source in order to estimate the poi
Publikováno v:
Proceedings of the International Astronomical Union. 8:176-177
In order to answer this question, we examine the relationship between the two sites of maser activity in G357.96-0.16. We also propose future observations for examining the dust properties of this interesting region of massive star formation.
Autor:
Tui Britton, Maxim Voronkov
Publikováno v:
Proceedings of the International Astronomical Union. 8:282-283
The bright 25 GHz series of methanol masers is formed in highly energetic regions of massive star formation and provides a natural signpost of shocked gas surrounding newly forming stars. A systematic survey for the 25 GHz masers has only recently be