Zobrazeno 1 - 10
of 42
pro vyhledávání: '"S. J. Meatheringham"'
Autor:
Ralph C. Bohlin, Peter R. Wood, J. P. Harrington, S. J. Meatheringham, Holland C. Ford, Stephen P. Maran, E. Vassiliadis, Michael A. Dopita, Theodore P. Stecher
Publikováno v:
The Astrophysical Journal. 503:253-277
We present the continuation of our analysis of narrowband [O III] images, obtained using the Hubble Space Telescope (HST), of planetary nebulae (PNs) in the Magellanic Clouds. Six objects, five in the Large Magellanic Cloud, are observed as part of t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4834144059b4a88b43ff0ed95d808b2e
https://doi.org/10.1086/305969
https://doi.org/10.1086/305969
Autor:
Stephen P. Maran, J. P. Harrington, Ralph C. Bohlin, S. J. Meatheringham, Peter R. Wood, Holland C. Ford, Theodore P. Stecher, E. Vassiliadis, Michael A. Dopita
Publikováno v:
The Astrophysical Journal Supplement Series. 114:237-261
The Faint Object Spectrograph on board the Hubble Space Telescope (HST) is used to obtain spectra in the wavelength range λλ1150-4800 of three planetary nebulae in the Small Magellanic Cloud and 10 planetary nebulae in the Large Magellanic Cloud. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7a81f7bef78d0b393328c6be0f926656
https://doi.org/10.1086/313071
https://doi.org/10.1086/313071
Autor:
Ralph C. Bohlin, S. J. Meatheringham, Theodore P. Stecher, Holland C. Ford, J. P. Harrington, E. Vassiliadis, Peter R. Wood, Stephen P. Maran, Michael A. Dopita
Publikováno v:
The Astrophysical Journal. 474:188-204
A photoionization analysis of Hubble Space Telescope UV and ground-based optical spectrophotometry is given for eight more planetary nebulae (PNs) in the Large Magellanic Cloud (LMC). This allows the central stars to be placed accurately on the H-R d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::51867ed9fa9702e7104bc8db6a1d4c16
https://doi.org/10.1086/303444
https://doi.org/10.1086/303444
Autor:
M. A. Dopita, P. R. Wood, S. J. Meatheringham, E. Vassiliadis, R. C. Bohlin, H. C. Ford, J. P. Harrington, T. P. Stecher, S. P. Maran
Publikováno v:
Symposium - International Astronomical Union. 180:417-427
We present the results of our major HST study of the evolution of PN in the Magellanic Clouds. This consists of imaging studies in [O III] and FOS UV spectroscopy. These data are then used in theoretical photoionisation models in conjuction with grou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c73fbb6a7d6a25caca33b2c63d152f1
https://doi.org/10.1017/s0074180900131675
https://doi.org/10.1017/s0074180900131675
Publikováno v:
Publications of the Astronomical Society of Australia. 12:244-247
The Figaro data reduction system was originally written for DEC VAXes running VMS, and little attention was paid to making it portable. Recently, however, a cooperative effort between the AAO, MSSSO, UNSW, the UK Starlink network and Caltech has resu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3cc47ed94725326b261ed361d0e78b4a
https://doi.org/10.1017/s1323358000020336
https://doi.org/10.1017/s1323358000020336
Autor:
S. J. Meatheringham
Publikováno v:
Symposium - International Astronomical Union. 148:89-95
The Small and Large Magellanic Clouds (SMC, LMC) are of considerable interest from a kinematical viewpoint. The tidal interation of the Clouds with each other and with the Galaxy appears to have been quite significant in recent times (Murai & Fujimot
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e64bf918e67de92891123a82c903b87c
https://doi.org/10.1017/s0074180900200077
https://doi.org/10.1017/s0074180900200077
Autor:
M. A. Dopita, S. J. Meatheringham, Steven N. Shore, R. Sutherland, S. G. Starrfield, George Sonneborn, Robert Williams
Publikováno v:
New Aspects of Magellanic Cloud Research ISBN: 9783540564324
Nova LMC 1990A was a very fast Ne-O-Mg nova, for which a particularly dense coverage of spectral observation in both the UV and optical was obtained. The data for the nebular phase were subjected to an analysis by the photoionisation modelling code M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::26221960649706d92dcd86b20c6979e5
https://doi.org/10.1007/3-540-56432-2_195
https://doi.org/10.1007/3-540-56432-2_195
Autor:
E. Vassiliadis, Ralph C. Bohlin, Theodore P. Stecher, Michael A. Dopita, Stephen P. Maran, Holland C. Ford, J. P. Harrington, Peter R. Wood, S. J. Meatheringham
Publikováno v:
Planetary Nebulae ISBN: 9780792348931
We present the results of our major HST study of the evolution of PN in the Magellanic Clouds. This consists of imaging studies in [O III] and FOS UV spectroscopy. These data are then used in theoretical photoionisation models in conjuction with grou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::de6e42515f344e193335097fe9dca919
https://doi.org/10.1007/978-94-011-5244-0_203
https://doi.org/10.1007/978-94-011-5244-0_203
Autor:
J. P. Harrington, Holland C. Ford, Peter R. Wood, Ralph C. Bohlin, S. J. Meatheringham, Theodore P. Stecher, E. Vassiliadis, S. R Maran, Michael A. Dopita
Publikováno v:
Planetary Nebulae ISBN: 9780792348931
The majority of planetary nebulae (PNe) at the distance of the Magellanic Clouds typically subtend 1 arcsec or less on the sky. The Planetary Camera onboard the Hubble Space Telescope has a scale of 0.044 arcsec per pixel and is therefore ideal to us
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c0863363e77a921a4b494ec434d09fdd
https://doi.org/10.1007/978-94-011-5244-0_215
https://doi.org/10.1007/978-94-011-5244-0_215
Autor:
Michael A. Dopita, S. J. Meatheringham, Theodore P. Stecher, Ralph C. Bohlin, Peter R. Wood, Holland C. Ford, J. P. Harrington, Stephen P. Maran
Publikováno v:
Planetary Nebulae ISBN: 9780792324409
We have obtained Hubble Space Telescope (HST) Planetary Camera (PC) images of a number of Magellanic Cloud planetary nebulae. The objects, except for SMP 83 were observed as part of the Cycle I GO program. The observations were made in the [O III] λ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::96fe169475c3a5c9a46de5281712bebb
https://doi.org/10.1007/978-94-011-2088-3_84
https://doi.org/10.1007/978-94-011-2088-3_84