Zobrazeno 1 - 10
of 38
pro vyhledávání: '"I. R. Tuohy"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 265:926-940
We report the discovery of a cataclysmic variable that was detected as an X-ray source by the HEAO-1 modulation collimator. The spectrum is typical of a weak-lined nova-like system, with moderately strong He II λ4686-A emission (∼0.3 Hβ) and a ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9d91d8b1f31bdfcebb8da9583999e3e0
https://doi.org/10.1093/mnras/265.4.926
https://doi.org/10.1093/mnras/265.4.926
Autor:
I. R. Tuohy, Ron Remillard, David A. Schwartz, Roger Brissenden, E. Rosenthal, D. A. H. Buckley
Publikováno v:
The Astrophysical Journal. 396:668
The evolution of the emission-line Star S-154, between February and December 1988, from a low-excitation 'Fe II star' into a high-excitation state that resembles symbiotic stars, is traced. It is inferred that the spectral type of central stars do no
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::acb409c7fab4c4a1f158417312625c6c
https://doi.org/10.1086/171747
https://doi.org/10.1086/171747
Autor:
D. A. H. Buckley, I. R. Tuohy
Publikováno v:
The Astrophysical Journal. 349:296
Optical spectroscopic and photometric observations of the hard X-ray-emitting HEAO 1 cataclysmic variable, H0534 - 581 are discussed. From the analysis of Exosat time series data, spectroscopic periods at 6 and 2.1 hr are identified as the orbital an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72cba6d00ec9b5ad729e77b277230ba3
https://doi.org/10.1086/168314
https://doi.org/10.1086/168314
Autor:
I. R. Tuohy
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 174:45P-50P
The 4.8 second X-ray pulsations from Centaurus X-3 were monitored by the MSSL collimated proportional counter on board Ariel-5 between 18-27 January 1975. Analysis of the source Doppler effect shows that the pulsation period of Cen X-3 decreased by 3
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b07c0c8d1f9844fd47e49e18d1719911
https://doi.org/10.1093/mnras/174.1.45p
https://doi.org/10.1093/mnras/174.1.45p
Publikováno v:
Symposium - International Astronomical Union. 101:559-565
We report the optical identification of four Balmer-dominated supernova remnants (SNRs) in the Large Magellanic Cloud. Both the Balmer-dominated spectra and the presence of a broad Hα component in one remnant can be understood in terms of a very hig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::392d2ba25cb891c314aae4e8ab708d07
https://doi.org/10.1017/s0074180900034434
https://doi.org/10.1017/s0074180900034434
Publikováno v:
Astrophysics and Space Science. 131:601-606
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4144c8313e9a99bef03a1908dff27638
https://doi.org/10.1007/bf00668144
https://doi.org/10.1007/bf00668144
Publikováno v:
Publications of the Astronomical Society of Australia. 6:186-194
A broad-band (2-190 keV) Australian X-ray satellite could provide a spectral sensitivity substantially better than HEAO-1 or any presently approved spacecraft. It would be virtually unique by providing simultaneously data over a wide energy range wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7c931780b859ad7ecaab3fa1a1ac7ff7
https://doi.org/10.1017/s1323358000018063
https://doi.org/10.1017/s1323358000018063
Publikováno v:
Symposium - International Astronomical Union. 101:541-549
Optical identifications of 32 X-ray sources in the Magellanic Clouds confirm that they are SNRs. They are separated into four classes: the evolved, the oxygen-rich, the Balmer-dominated and the Crab-like. High velocity HI emission is observed from an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::05c13d5dd38687233ba463aa96e2ecbf
https://doi.org/10.1017/s0074180900034410
https://doi.org/10.1017/s0074180900034410
The Peculiar X-ray Morphology of the SNR G292.0+1.8 : Evidence for an Asymmetric Supernova Explosion
Autor:
D. H. Clark, I. R. Tuohy
Publikováno v:
Symposium - International Astronomical Union. 101:153-158
A high resolution X-ray image from the Einstein Observatory of the young supernova remnant G292.0+1.8 (MSH11–54), previously noted as peculiar in terms of its spectral and morphological properties at optical and radio wavelengths, also shows an unu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c7e122558556db0584257bf5a8b630e4
https://doi.org/10.1017/s0074180900033817
https://doi.org/10.1017/s0074180900033817
Autor:
A. M. Cruise, I. R. Tuohy
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 171:33P-39P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::98f187a56ea6ca4f455c9a0d8930a616
https://doi.org/10.1093/mnras/171.1.33p
https://doi.org/10.1093/mnras/171.1.33p