# CWISEP J193518.59$-$154620.3: An Extremely Cold Brown Dwarf in the Solar   Neighborhood Discovered with CatWISE

**Authors:** Federico Marocco (1,2), Dan Caselden (3), Aaron M. Meisner (4), J., Davy Kirkpatrick (2), Edward L. Wright (5), Jacqueline K. Faherty (6),, Christopher R. Gelino (2), Peter R. M. Eisenhardt (1), John W. Fowler (7),, Michael C. Cushing (8), Roc M. Cutri (2), Nelson Garcia (2), Thomas H., Jarrett (9), Renata Koontz (10,1), Amanda Mainzer (1), Elijah J. Marchese, (10,1), Bahram Mobasher (10), David J. Schlegel (11), Daniel Stern (1), Harry, I. Teplitz (2) ((1) Jet Propulsion Laboratory, Caltech, USA, (2) IPAC,, Caltech, USA, (3) Gigamon ATR, USA, (4) National Optical Astronomy, Observatory, USA, (5) UCLA, USA, (6) American Museum of Natural History, USA,, (7) 230 Pacific St., Apt. 205, Santa Monica, CA, USA, (8) University of, Toledo, USA, (9) University of Cape Town, USA, (10) UC Riverside, USA, (11), Lawrence Berkeley National Laboratory, USA)

arXiv: 1906.08913 · 2019-08-14

## TL;DR

This paper reports the discovery of an extremely cold brown dwarf in the solar neighborhood, identified through the CatWISE catalog, with follow-up observations indicating it has one of the lowest temperatures among known brown dwarfs.

## Contribution

The study introduces a new nearby, ultra-cold brown dwarf with detailed photometric analysis and proper motion measurements, expanding knowledge of the coldest substellar objects.

## Key findings

- Effective temperature estimated between 270-360 K.
- Distance estimated between 5.6-10.9 parsecs.
- Proper motion indicates low tangential velocity.

## Abstract

We present the discovery of an extremely cold, nearby brown dwarf in the solar neighborhood, found in the CatWISE catalog (Eisenhardt et al., in prep.). Photometric follow-up with Spitzer reveals that the object, CWISEP J193518.59-154620.3, has ch1$-$ch2 = 3.24$\,\pm\,$0.31 mag, making it one of the reddest brown dwarfs known. Using the Spitzer photometry and the polynomial relations from Kirkpatrick et al. (2019) we estimate an effective temperature in the $\sim$270--360 K range, and a distance estimate in the 5.6$-$10.9 pc range. We combined the WISE, NEOWISE, and Spitzer data to measure a proper motion of $\mu_\alpha \cos \delta = 337\pm69$ mas yr$^{-1}$, $\mu_\delta = -50\pm97$ mas yr$^{-1}$, which implies a relatively low tangential velocity in the range 7$-$22 km s$^{-1}$.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1906.08913/full.md

## References

42 references — full list in the complete paper: https://tomesphere.com/paper/1906.08913/full.md

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Source: https://tomesphere.com/paper/1906.08913