# Low mass visual binaries in the solar neighbourhood: The case of HD141272

## TL;DR

This study reports the discovery of a new stellar companion to HD141272, confirming its co-movement and characterizing its spectral type and mass, contributing to understanding stellar multiplicity in the solar neighborhood.

## Contribution

First detection of a co-moving stellar companion to HD141272 using multi-epoch imaging, spectroscopy, and photometry, advancing knowledge of nearby stellar systems.

## Key findings

- Discovered a co-moving M3+-0.5V companion at 350 AU from HD141272.
- Confirmed the companion's spectral type and mass as a ~0.26 M_sun dwarf.
- System is consistent with the ZAMS, ruling out pre-main sequence status.

## Abstract

We search for stellar and substellar companions of young nearby stars to investigate stellar multiplicity and formation of stellar and substellar companions. We detect common proper-motion companions of stars via multi-epoch imaging. Their companionship is finally confirmed with photometry and spectroscopy. Here we report the discovery of a new co-moving (13 sigma) stellar companion ~17.8 arcsec (350 AU in projected separation) north of the nearby star HD141272 (21 pc). With EMMI/NTT optical spectroscopy we determined the spectral type of the companion to be M3+-0.5V. The derived spectral type as well as the near infrared photometry of the companion are both fully consistent with a 0.26+-0.07 Msol dwarf located at the distance of HD141272 (21 pc). Furthermore the photometry data rules out the pre-main sequence status, since the system is consistent with the ZAMS of the Pleiades.