期刊
ASTRONOMY & ASTROPHYSICS
卷 622, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201834688
关键词
binaries: close; stars: low-mass; stars: pre-main sequence; techniques: imaging spectroscopy; planets and satellites: detection
资金
- Knut and Alice Wallenberg foundation
- Progetti Premiali funding scheme of the Italian Ministry of Education, University, and Research
- MEXT/JSPS KAKENHI [17K05399, 18H05442, 15H02063, 22000005]
- Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan [2302, 23103002]
- Grants-in-Aid for Scientific Research [18H05442, 17K05399] Funding Source: KAKEN
We present SCExAO/CHARIS 1.1-2.4 mu m integral field direct spectroscopy of the young HIP 79124 triple system. HIP 79124 is a member of the Scorpius-Centaurus association, consisting of an A0V primary with two low-mass companions at a projected separation of <1 ''. Thanks to the high quality wavefront corrections provided by SCExAO, both companions are decisively detected without the employment of any PSF-subtraction algorithm to eliminate quasi-static noise. The spectrum of the outer C object is very well matched by Upper Scorpius M4 +/- 0.5 standard spectra, with a T-eff = 2945 +/- 100 K and a mass of similar to 350 M-Jup. HIP 79124 B is detected at a separation of only 180 mas in a highly-correlated noise regime, and it falls in the spectral range M6 +/- 0.5 with T-eff = 2840 +/- 190 K and similar to 100 M-Jup. Previous studies of stellar populations in Sco-Cen have highlighted a discrepancy in isochronal ages between the lower-mass and higher-mass populations. This could be explained either by an age spread in the region, or by conventional isochronal models failing to reproduce the evolution of low-mass stars. The HIP 79124 system should be coeval, and therefore it provides an ideal laboratory to test these scenarios. We place the three components in a color-magnitude diagram and find that the models predict a younger age for the two low-mass companions (similar to 3 Myr) than for the primary star (similar to 6 Myr). These results imply that the omission of magnetic effects in conventional isochronal models inhibit them from reproducing early low-mass stellar evolution, which is further supported by the fact that new models that include such effects provide more consistent ages in the HIP 79124 system.
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