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- W1656197112 abstract "Near infrared photometric data which identify the embedded low-luminosity object SSV 13 (HH 7-11 IRS) as a variable are presented. At 2.2 μm, the source has recently brightened by as much as about one magnitude within only one year. The accompanying changes in colour are not directly compatible with those expected from observed interstellar extinction curves. Whereas the observed source spectrum at any one instant cannot be represented by a single-temperature blackbody, the distribution of the surplus flux in the bright state is well fit by a single blackbody emitter" @default.
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- W1656197112 date "1992-01-01" @default.
- W1656197112 modified "2023-09-26" @default.
- W1656197112 title "The infrared variability of SSV 13." @default.
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