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An unusual high-redshift object discovered with the Hubble Space Telescope : peculiar starburst galaxy or new gravitational lens?
DOI: 10.1093/mnras/270.1.L63 Bibcode: 1994MNRAS.270L..63G

Glazebrook, K.; Griffiths, R.; Ellis, R. +2 more

We report the discovery of an object with a very peculiar structure, using observations from the refurbished Hubble Space Telescope (HST) as part of the Medium-Deep Survey project. The object includes four compact blue components arranged around an extended red component, with mutual separations of <1 arcsec. Using a ground-based spectrum as an…

1994 Monthly Notices of the Royal Astronomical Society
eHST 12
3 Puppis : a peculiar object with infrared excess.
DOI: 10.1093/mnras/266.1.203 Bibcode: 1994MNRAS.266..203R

Rovero, Adrian C.; Ringuelet, Adela E.

We present a model that accounts for the UV, photographic, and IR observations of 3 Puppis. The model consists of a binary system in which the primary is an A supergiant with a mild chromosphere; the primary fills its Roche lobe. The velocity law in the extended atmosphere, which is responsible for the density distribution of the gas, and a chromo…

1994 Monthly Notices of the Royal Astronomical Society
IUE 12
Optical and UV spectroscopy towards stars in the direction of the Cohen high-velocity H I stream.
DOI: 10.1093/mnras/270.3.597 Bibcode: 1994MNRAS.270..597K

Dufton, P. L.; Keenan, F. P.; Bates, B. +2 more

We present high-resolution, high signal-to-noise ratio optical spectra and UV spectra obtained with lUE for several stars that lie within and adjacent to the Cohen high- velocity (Hv) stream, which is considered by Cohen to lie within 300 pc. From spectral classifications, published photometry and LTE model atmosphere analysis of our stellar spect…

1994 Monthly Notices of the Royal Astronomical Society
IUE 11
A non-thermal radio/optical/X-ray source in PKS 2316-423.
DOI: 10.1093/mnras/266.3.669 Bibcode: 1994MNRAS.266..669C

Fabian, A. C.; Crawford, C. S.

We report observations of PKS 2316-423 in the ultraviolet and with the ROSAT HRI, where it appears as a bright point source. Optical spectroscopy reveals weak emission lines and a strong, excess blue continuum that is centrally concentrated. The combined optical- ultraviolet continuum spectrum cannot be fitted by any simple combination of a main-s…

1994 Monthly Notices of the Royal Astronomical Society
IUE 11
Pulsational Activity on Ik-Pegasi
DOI: 10.1093/mnras/267.4.1045 Bibcode: 1994MNRAS.267.1045W

Kellett, B. J.; Lloyd, C.; Smalley, B. +1 more

High-time-resolution photometry of millimagnitude precision using the Fine Error Sensor on board the International Ultraviolet Explorer is presented. A few hours of data, when subjected to an optimal (Bayesian) analysis, reveal two pulsational frequencies in the star 1K Peg A, one of which was not previously known. A fit to the empirical P-L-C rel…

1994 Monthly Notices of the Royal Astronomical Society
IUE 8
The Latest Spectral Peregrinations of Rx-Puppis
DOI: 10.1093/mnras/268.2.561 Bibcode: 1994MNRAS.268..561I

Ivison, R. J.; Seaquist, E. R.

We present centimetre- and millimetre-wave continuum measurements of the symbiotic binary system RX Puppis. These suggest that RX Pup has returned to a state of low excitation after more than a decade of activity. Although the overall optical brightness has not altered substantially during the past two years, recent low-resolution ultraviolet and …

1994 Monthly Notices of the Royal Astronomical Society
IUE 5