Zobrazeno 1 - 10
of 48
pro vyhledávání: '"S. M. G. Hughes"'
Autor:
S. M. G. Hughes
Publikováno v:
International Astronomical Union Colloquium. 136:352-355
A series of 40 HST WFC exposures in v (F555W) and i (F785LP) have been obtained of two fields in M81, in order to search for Cepheid variables. This has provided an ideal opportunity to compare how the photometry programs DoPHOT and DAOPHOT cope with
Publikováno v:
Symposium - International Astronomical Union. 148:259-265
Until recently, surveys for variable stars in the Magellanic Clouds were carried out in blue and visual passbands, but these passbands are not ideal for finding very cool stars such as long-period variables (LPVs). Consequently, the early surveys gen
We extend the work developed in previous papers on microlensing with a selection of variable stars. We use the Pixel Method to select variable stars on a set of 2.5 x 10**6 pixel light curves in the LMC Bar presented elsewhere. The previous treatment
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::613893f7d218e814cac6e75bf3ed9beb
http://arxiv.org/abs/astro-ph/0102089
http://arxiv.org/abs/astro-ph/0102089
Autor:
P. R. Wood, M. S. Bessell, S. M. G. Hughes, A. R. Hyland, J. B. Whiteoak, F. F. Gardner, R. E. Otrupcek
Publikováno v:
The Magellanic Clouds ISBN: 9780792311119
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ef866614ff88f4be96a32c326efc374e
https://doi.org/10.1007/978-94-011-3432-3_103
https://doi.org/10.1007/978-94-011-3432-3_103
Autor:
S. M. G. Hughes
Publikováno v:
International Astronomical Union Colloquium. 155:258-259
As part of the Extragalactic Distance Scale Key Project, the Hubble Space Telescope has been used to identify Cepheids in M100, M101 and NGC925, and to measure distances derived from the Cepheid PL relation. For M100, the distance of 17.1 ± 1.8 Mpc
Autor:
A. R. Hyland, F. F. Gardner, Robina E. Otrupcek, Peter R. Wood, J. B. Whiteoak, S. M. G. Hughes, M. S. Bessell
Publikováno v:
Symposium - International Astronomical Union. 148:386-387
In 1985 we began a search for OH/IR objects in the Magellanic Clouds. The first detection was reported by Wood, Bessell & Whiteoak (1986). Subsequent searches have yielded several of these objects and other highly-evolved stars obscured by thick circ
Autor:
F. F. Gardner, J. B. Whiteoak, Michael S. Bessell, A. R. Hyland, S. M. G. Hughes, Peter R. Wood
Publikováno v:
The Astrophysical Journal. 397:552
A sample of IRAS point sources in the Magellanic Clouds has been searched for 1612 MHz maser emission and for infrared emission at JHKL'. Six point sources, all in the LMC, are found to be OH masers while 19 have strong infrared emission typical of e
Publikováno v:
Publications of the Astronomical Society of Australia. 5:547-552
Carbon, nitrogen and oxygen are of interest for stellar and galactic evolution for four main reasons. Firstly, they comprise most of the mass of elements heavier than helium, so their abundance reflects the bulk of chemical enrichment. Secondly, all
Autor:
Peter R. Wood, S. M. G. Hughes
Publikováno v:
Publications of the Astronomical Society of Australia. 7:147-150
A photometric survey of a central region of the LMC has been undertaken to obtain a magnitude and colour limited sample of bright asymptotic giant branch (AGB) stars; the stars were selected from V and Ic plates taken by the UK Schmidt Telescope Unit
Publikováno v:
Fortschritte der Physik / Progress of Physics; Dec2023, Vol. 71 Issue 12, p1-17, 17p