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Title: Validation of Elemental and Isotopic Abundances in Late-M Spectral Types with the Benchmark HIP 55507 AB System
Abstract

M dwarfs are common host stars to exoplanets but often lack atmospheric abundance measurements. Late-M dwarfs are also good analogs to the youngest substellar companions, which share similarTeff∼ 2300–2800 K. We present atmospheric analyses for the M7.5 companion HIP 55507 B and its K6V primary star with Keck/KPIC high-resolution (R∼ 35,000)K-band spectroscopy. First, by including KPIC relative radial velocities between the primary and secondary in the orbit fit, we improve the dynamical mass precision by 60% and findMB=88.03.2+3.4MJup, putting HIP 55507 B above the stellar–substellar boundary. We also find that HIP 55507 B orbits its K6V primary star witha=383+4au ande= 0.40 ± 0.04. From atmospheric retrievals of HIP 55507 B, we measure [C/H] = 0.24 ± 0.13, [O/H] = 0.15 ± 0.13, and C/O = 0.67 ± 0.04. Moreover, we strongly detect13CO (7.8σsignificance) and tentatively detectH218O(3.7σsignificance) in the companion’s atmosphere and measure12CO/13CO=9822+28andH216O/H218O=24080+145after accounting for systematic errors. From a simplified retrieval analysis of HIP 55507 A, we measure12CO/13CO=7916+21andC16O/C18O=28870+125for the primary star. These results demonstrate that HIP 55507 A and B have consistent12C/13C and16O/18O to the <1σlevel, as expected for a chemically homogeneous binary system. Given the similar flux ratios and separations between HIP 55507 AB and systems with young substellar companions, our results open the door to systematically measuring13CO andH218Oabundances in the atmospheres of substellar or even planetary-mass companions with similar spectral types.

 
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PAR ID:
10489028
Author(s) / Creator(s):
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Publisher / Repository:
DOI PREFIX: 10.3847
Date Published:
Journal Name:
The Astrophysical Journal
Volume:
962
Issue:
1
ISSN:
0004-637X
Format(s):
Medium: X Size: Article No. 10
Size(s):
Article No. 10
Sponsoring Org:
National Science Foundation
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