Infrared Study of a Low-mass Star-forming Region L1251B

  • Choi, Yunhee (Kyung Hee University) ;
  • Lee, Jeong-Eun (Kyung Hee University) ;
  • Bergin, Edwin A. (University of Michigan) ;
  • Blake, Geoffrey A. (California Institute of Technology) ;
  • Boogert, A.C. Adwin (NASA Ames Research Center) ;
  • Francesco, James Di (National Research Council) ;
  • Evans, Neal J. II (University of Texas at Austin) ;
  • Pontoppidan, Klaus M. (Space Telescope Science Institute) ;
  • Sargent, Annelia I. (California Institute of Technology)
  • Published : 2016.10.12

Abstract

A low-mass star-forming region, L1251B, is an excellent example of a small and nearby group of protostellar objects. L1251B has been mapped spectroscopically with the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. IRS has provided mid-IR emission lines (e.g., [Fe II], [Ne II], and ro-vibrational H2) and absorption features of CO2 and H2O ice in studying the physical state of the ionized gas and the material residing in the circumstellar environments. We will present the distribution of outflows and ice components in L1251B.

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