A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2019; you can also visit the original URL.
The file type is application/pdf.
A Deep Survey of Infrared Sources in the Field of the Small Magellanic Cloud
1985
Publications Astronomical Society of Australia
Preserved Fulltext
AbstractWe present a survey at J (1.25μm) and K (2.2μm) of 36 arcmin2in the Bar and Inner Wing of the Small Magellanic Cloud. The (J-K) colour – bolometric magnitude diagram is constructed and compared with theory. For the first time a sparsely populated region of the diagram separating proposed carbon stars from oxygen rich stars has been identified. In addition large numbers of red sources have been found apparently fainter than the accepted limit for carbon star formation. These include
doi:10.1017/s1323358000026643
fatcat:ddxmxmwwc5fw5h2a5fie4rzp2q