Photoelectric observations were made of four N stars (HD 51208, HD 75021, V 1942 Sgr, and RU Vir) at careful1y chosen discrete wavelengths between 7000 |AA a n d 11000 |AA with 30 |AA bandpass width. Their effective temperatures have been derived by fitting the black-body radiation curve to the observed continuum intensities at 7800 |AA , 9000 |AA a n d 10800 |AA . The resulting temperature ranges from 2500˚ K t o 2900 ˚ K . . It is probable that almost all the N stars belong to this range of temperature. However, the temperatures of very red N stars can not be well determined due to large variability and redistribution of their radiation energy arising from the graphite shells around them.

Abstract
Ⅰ. 序論
Ⅱ. 觀測
Ⅲ. N星의 溫度
Ⅳ. 結論
參考文獻

• 李榮範(Attached High School, College Education, Seoul National University) | Youngbom Lee