Strength of the radiation of the young massive star G358 as a function of the wavelength
Date
Strength of the radiation of the young massive star G358 as a function of the wavelength. Dots mark measured values from FIFI-LS/SOFIA (red & green) and PACS/Herschel satellite (blue) and lines the modeled emission of the object. The colors mark points in time, with blue meaning before the stochastic accretion event, red during (SOFIA flight 1) and green, 18 months after (SOFIA flight 2).
Credit
Stecklum et al. 2021
Image Number
SCI2021_008
Additional Information
Strength of the radiation of the young massive star G358 as a function of the wavelength
Instrument
FIFI-LS
Location
United States
More Information
