1. SOFIA/HAWC polarimetry of low-mass YSOs and their environs

2. SHARP

3. SOFIA/HAWC polarimetry of low-mass YSOs and their environs SHARP Class 0

4. - molecular clouds have ordered B-fields - what is energy density, compared with… gravity? turbulence? rotation? - see Crutcher 2004 review article (CF, Zeeman) - if fields are energetically important, they probably affect dynamical collapse of cores

5. Crutcher 2006 isolated, lo-mass SF

6. Crutcher 2006 1 - few thousand AU isolated, lo-mass SF

7. Crutcher 2006 1 - few thousand AU isolated, lo-mass SF

8. low-mass pinch in NGC 1333 IRAS4A (Girart, Rao, & Marrone 2006) Class II YSO

9. low-mass pinch in NGC 1333 IRAS4A (Girart, Marrone, & Rao 2006) Class II YSO

10. low-mass pinch in NGC 1333 IRAS4A (Girart, Marrone, & Rao 2006) Class II YSO why not more lo-mass pinches? faint, small why not more cases of B parallel to outflow? maybe because very uniform fields are rare

11. more typical case is this prestellar core… (Kirk, Ward-Thompson, & Crutcher 2006) …to find correlation between outflow and field, need to map field right where star is forming… within a few thousand AU. will attempt with SHARP…

12. SHARP: 9 arcsec beam at 350 microns 9 arcsec is 1800 AU at 200 pc (SCUBA polarimeter had 14 arcsec) In comparison with 800 micron maps from the SCUBA polarimeter 350 micron observations are relatively more sensitive to warm dust near to the protostar,

13. criteria used for the Class 0 target list distance < 400 pc distance to nearest neighbor must be > 10,000 AU preference for outflow axis nearly parallel to plane of sky

14. criteria used for the Class 0 target list distance < 400 pc distance to nearest neighbor must be > 10,000 AU preference for outflow axis nearly parallel to plane of sky

15. target list of Class 0 YSOs for winter season (developed mainly by Brenda Matthews and Jackie Davidson)

16. goals of SHARP survey of Class 0 YSOs 1. test for correlation of projected field direction with projected outflow direction 2. look for pinches (beam ~1800 AU @ 200 pc) Both find  < 2 for most TTS disks

17. goals of SOFIA/HAWCpol survey of Class 0 and Class I YSOs 1. test for correlation of projected field direction with projected outflow direction 2. look for pinches (beam ~ 900 AU @ 200 pc; 50  m) better ability to isolate the warmer inner regions can trace evolution of B-field get a 3D view