Infrared emission and star formation in the central regions of the galaxy IC 342
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Becklin, E. E.↗
Engineering topics
Publications and source records attributed to Sellgren, K..
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Observations of Algol (Beta Persei) at 10 microns are presented which are of relevance to the system's behavior around the time of its secondary minimum. No evidence is found for a significant excess at 10 microns. The data show a smooth decline by 0.3 mag which starts at about phase 0.42, while the limited data obtained at phases greater than 0.50 are consistent with a symmetrical curve about phase 0.50.