An Investigation of New Brown Dwarf Spectral Binary Candidates From the Backyard Worlds: Planet 9 Citizen Science Initiative

被引:1
|
作者
Bravo, Alexia [1 ]
Schneider, Adam C. [1 ]
Gagliuffi, Daniella Bardalez [2 ]
Burgasser, Adam J. [3 ]
Meisner, Aaron M. [4 ]
Kirkpatrick, J. Davy [5 ]
Faherty, Jacqueline K. [6 ]
Kuchner, Marc J. [7 ]
Caselden, Dan [6 ]
Sainio, Arttu [8 ]
Hamlet, Les [8 ]
机构
[1] US Naval Observ, Flagstaff Stn, 10391 West Naval Observ Rd, Flagstaff, AZ 86005 USA
[2] Amherst Coll, Dept Phys & Astron, 25 East Dr, Amherst, MA 01003 USA
[3] Univ Calif San Diego, Dept Astron & Astrophys, La Jolla, CA 92093 USA
[4] NSFs Natl Opt Infrared Astron Res Lab, 950 N Cherry Ave, Tucson, AZ 85719 USA
[5] CALTECH, IPAC, Mail Code 100-22,1200 E Calif Blvd, Pasadena, CA 91125 USA
[6] Amer Museum Nat Hist, Dept Astrophys, Cent Pk West & 79th St, New York, NY 10024 USA
[7] NASA, Exoplanets & Stellar Astrophys Lab, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA
[8] Backyard Worlds Planet 9, Tucson, AZ USA
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
SPITZER FOLLOW-UP; T-DWARF; LOW-MASS; PHYSICAL-PROPERTIES; SPEX SPECTROSCOPY; ADAPTIVE OPTICS; COOL NEIGHBORS; DISCOVERY; 2MASS; SEARCH;
D O I
10.3847/1538-3881/acffc1
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present three new brown dwarf spectral-binary candidates: CWISE J072708.09-360729.2, CWISE J103604.84-514424.4, and CWISE J134446.62-732053.9, discovered by citizen scientists through the Backyard Worlds: Planet 9 project. Follow-up near-infrared spectroscopy shows that each of these objects is poorly fit by a single near-infrared standard. We constructed binary templates and found significantly better fits, with component types of L7+T4 for CWISE J072708.09-360729.2, L7+T4 for CWISE J103604.84-514424.4, and L7+T7 for CWISE J134446.62-732053.9. However, further investigation of available spectroscopic indices for evidence of binarity and large amplitude variability suggests that CWISE J072708.09-360729.2 may instead be a strong variability candidate. Our analysis offers tentative evidence and characterization of these peculiar brown dwarf sources, emphasizing their value as promising targets for future high-resolution imaging or photometric variability studies.
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页数:7
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