TY - JOUR
T1 - HIP 67506 C
T2 - MagAO-X confirmation of a new low-mass stellar companion to HIP 67506 A
AU - Pearce, Logan A.
AU - Males, Jared R.
AU - Haffert, Sebastiaan Y.
AU - Close, Laird M.
AU - Long, Joseph D.
AU - McLeod, Avalon L.
AU - Knight, Justin M.
AU - Hedglen, Alexander D.
AU - Weinberger, Alycia J.
AU - Guyon, Olivier
AU - Kautz, Maggie
AU - Van Gorkom, Kyle
AU - Lumbres, Jennifer
AU - Schatz, Lauren
AU - Rodack, Alex
AU - Gasho, Victor
AU - Kueny, Jay
AU - Foster, Warren
AU - Morzinski, Katie M.
AU - Hinz, Philip M.
N1 - Publisher Copyright:
© 2023 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society.
PY - 2023/5/1
Y1 - 2023/5/1
N2 - We report the confirmation of HIP 67506 C, a new stellar companion to HIP 67506 A. We previously reported a candidate signal at 2λ/D (240 mas) in L′ in MagAO/Clio imaging using the binary differential imaging technique. Several additional indirect signals showed that the candidate signal merited follow-up: significant astrometric acceleration in Gaia DR3, Hipparcos-Gaia proper motion anomaly, and overluminosity compared to single main-sequence stars. We confirmed the companion, HIP 67506 C, at 0.1 arcsec with MagAO-X in 2022 April. We characterized HIP 67506 C MagAO-X photometry and astrometry, and estimated spectral-type K7-M2; we also re-evaluated HIP 67506 A in light of the close companion. Additionally, we show that a previously identified 9 arcsec companion, HIP 67506 B, is a much further distant unassociated background star. We also discuss the utility of indirect signposts in identifying small inner working angle candidate companions.
AB - We report the confirmation of HIP 67506 C, a new stellar companion to HIP 67506 A. We previously reported a candidate signal at 2λ/D (240 mas) in L′ in MagAO/Clio imaging using the binary differential imaging technique. Several additional indirect signals showed that the candidate signal merited follow-up: significant astrometric acceleration in Gaia DR3, Hipparcos-Gaia proper motion anomaly, and overluminosity compared to single main-sequence stars. We confirmed the companion, HIP 67506 C, at 0.1 arcsec with MagAO-X in 2022 April. We characterized HIP 67506 C MagAO-X photometry and astrometry, and estimated spectral-type K7-M2; we also re-evaluated HIP 67506 A in light of the close companion. Additionally, we show that a previously identified 9 arcsec companion, HIP 67506 B, is a much further distant unassociated background star. We also discuss the utility of indirect signposts in identifying small inner working angle candidate companions.
KW - (stars:) binaries: visual
KW - methods: data analysis
KW - methods: observational
KW - planets and satellites: detection
KW - stars: statistics
UR - http://www.scopus.com/inward/record.url?scp=85160307854&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85160307854&partnerID=8YFLogxK
U2 - 10.1093/mnras/stad859
DO - 10.1093/mnras/stad859
M3 - Article
AN - SCOPUS:85160307854
SN - 0035-8711
VL - 521
SP - 4775
EP - 4784
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 3
ER -