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Silverstone, M. D.; Becklin, E. E.; Spangler, C.

doi:10.1023/a:1001179221922

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2001

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“…As far as possible, these FCS-based calibrations were cross-checked by comparing Henry et al 1996. (2) the method of calibration from the observed ISO and published IRAS backgrounds and a number of actual IRAS source measurements as described by Silverstone, Becklin, & Spangler (1997), Silverstone (2000), and Spangler et al (1999) and were found to be consistent. A more detailed discussion of the calibration comparisons is given in the Appendix.…”

Section: Observations and Resultsmentioning

confidence: 99%

Dusty Debris around Solar‐Type Stars: Temporal Disk Evolution

Spangler

Sargent

Silverstone

et al. 2001

ApJ

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167

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Using ISO-ISOPHOT, we carried out a survey of almost 150 stars to search for evidence of emission from dust orbiting young main-sequence stars, both in clusters and isolated systems. Over half of the detections are new examples of dusty stellar systems and demonstrate that such dust can be detected around numerous stars older than a few times 106 yr. Fluxes at 60 and either 90 or 100 km for the new excess sources together with improved Ñuxes for a number of IRAS-identiÐed sources are presented. Analysis of the excess luminosity relative to the stellar photosphere shows a systematic decline of this excess with stellar age consistent with a power-law index of [2.

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Section: Observations and Resultsmentioning

confidence: 99%