Search Publications

IUE observations of Large Magellanic Cloud members and detection of the 2,200 Å feature
DOI: 10.1038/276478a0 Bibcode: 1978Natur.276..478N

Nandy, K.; Morgan, D. H.

THE dominant feature in the UV spectra of reddened stars in our Galaxy is the broad absorption feature of interstellar origin, centred near 2,200 Å and having a halfwidth of 350 Å (ref. 1). The wavelength position of this feature and the correlation of its strength with other interstellar extinction parameters, for example, the visual colour exces…

1978 Nature
IUE 15
On the identification of celestial γ-ray sources
DOI: 10.1038/274346a0 Bibcode: 1978Natur.274..346M

Massaro, E.; Scarsi, L.

THE observations from COS B have provided a new and more detailed picture of the high energy γ-ray emission from the Galaxy. We discuss here the first catalogue with 13 localised sources which has been compiled1,2 and how the list should lengthen in the near future, as the data analysis progresses.

1978 Nature
COS-B 3
IUE observations of the eclipsing binary Epsilon Aurigae
DOI: 10.1038/276376a0 Bibcode: 1978Natur.276..376H

Hack, M.; Selvelli, P. L.

THE eclipsing binary Epsilon Aur is almost peculiar binary system and it has not been explained satisfactorily. We report here our observations of this system using the International Ultraviolet Explorer (IUE) collected at the Villafranca Satellite Tracking Station of the European Space Agency (SA).

1978 Nature
IUE 2
The International Ultraviolet Explorer (IUE)
DOI: 10.1038/275371a0 Bibcode: 1978Natur.275..371W

Wilson, R.

1978 Nature
IUE 1
International Ultraviolet Explorer to be launched this week
DOI: 10.1038/271299a0 Bibcode: 1978Natur.271..299S

Sharrock, Stuart

1978 Nature
IUE 0
New high energy gamma-ray sources observed by COS B
DOI: 10.1038/269494a0 Bibcode: 1977Natur.269..494H

Bignami, G. F.; Hermsen, W.; Masnou, J. L. +7 more

Results are reported for a search for gamma-ray sources based on data obtained by the COS B satellite. Ten previously unknown sources were discovered which appear to be galactic and which have typical gamma-ray luminosities of 10 to the 35th power erg/s above 100 MeV. The latitude distribution of the sources is taken as an immediate indication of …

1977 Nature
COS-B 164