Abstract

2004년 3월 25일부터 4일 동안 보현산천문대의 1.8m 망원경과 BOES(Bohyunsan Optical Echelle Spectrograph)를 사용하여 AG Vir의 고분산 분광관측을 수행하고, 전위상에 걸쳐 총 59개의 스펙트럼을 얻었다. 쌍성계의 시선속도를 얻기 위하여, 교차상관함수(CCF; Cross-Correlation Function) 와 선폭증가함수(BF; Broadening Function)를 관측된 스펙트럼의 분석에 사용하였다. 이때, 교차상관함수 분석을 통하여 주성의 시선속도만을 얻을수 있었던 반면, 선폭증가함수 분석을 통하여 두 성분별의 시선속도를 모두 구할 수 있었다. 우리는 분광 궤도요소(<TEX>$K_1=90.5km/s$</TEX>와 <TEX>$K_2=258.8km/s$</TEX>)와 Bell, Rainger, & Hilditch(1990)의 측광학적 해로부터 AG Vir의 절대 물리량을 다음과 같이 산출하였다. 즉, <TEX>$M_1:1.99M_\bigodot,\;M_2:0.62M_\bigodot,\; R_1=2.21R_\bigodot,\;R_2=1.36R_\bigodot,\;L_1=13.17L_\bigodot$</TEX>, 그리고 <TEX>$L_2=3.47L_\bigodot$</TEX>. 우리가 구한 각 성분별의 질량과 반경은 Bell, Rainger, & Hilditch(1990)의 값보다 더 크고, 광도 또한 더 밝다. 발표된 모든 시선속도곡선을 재분석한 결과, AG Vir의 시스템 속도는 약 <TEX>${\pm}8km/s$</TEX>의 비교적 큰 편차를 나타낸다. 그러나 이 변화가 Qian(2001)이 제안한 제3 천체의 광시간 효과에 의해 일어난다고 단정 지을 수 있는 근거를 찾을 수는 없었다. We performed a new high-resolution spectroscopy of AG Vir for 4 nights from 25 March 2004 using the BOES (Bohyunsan Optical Echelle Spectrograph) attached to the 1.8-m reflector at Bohyunsan Optical Astronomy Observatory, and obtained a total of 59 spectra where all orbital phases are covered. To get the radial velocities of the binary system, both method of the CCF (Cross-Co..elation Function)and the BF (Broadening Function) were applied to the analysis of all the observed spectra. From these, the CCF could calculate the radial velocities of the primary star alone, while the BF could determine those of the primary and the secondary components. New absolute dimensions were deduced with the combination of our spectroscopic orbital elements (<TEX>$K_1=90.5km/s$</TEX>와 <TEX>$K_2=258.8$</TEX>) and the photometric solutions of Bell, Rainger, & Hilditch (1990): <TEX>$A_1,=1.99M_\bigodot,\;M_2=0.62M_\bigodot,\;R_1=2.21R_\bigodot,\;R_2=1.36R_\bigodot,\;L_1=13.17L_\bigodot,\;and\;L_2=3.47L_\bigodot$</TEX>. Our absolute parameters are larger and brighter than those derived from Bell, Rainger, & Hilditch (1990). We re-analyzed all the previous radial-velocity curves of AG Vir and, as a result, can see that its system velocity scatters largely up to <TEX>${\pm}8km/s$</TEX>. However, we, at present, cannot determine this as the light-time effect due to the third body, which was suggested as a cause of the orbital period changes by Qian (2001).

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