HD 16754

HD 16754 is a binary or triple-star system in the constellation Eridanus. It has the Bayer designation s Eridani; HD 16754 is the designation from the Henry Draper catalogue. The system is visible to the naked eye as a faint point of light with an apparent visual magnitude of +4.74. It is located at a distance of approximately 132 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +18 km/s. The system is a member of the Columba association of co-moving stars.

HD 16754
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension 02h 39m 47.96544s
Declination −42° 53 30.3638
Apparent magnitude (V) +4.74
Characteristics
Spectral type A1 Vb + M2-5V + ?
B−V color index 0.061±0.003
Astrometry
Radial velocity (Rv)+18.0±4.2 km/s
Proper motion (μ) RA: +88.20 mas/yr
Dec.: −17.82 mas/yr
Parallax (π)24.7076 ± 0.3930 mas
Distance132 ± 2 ly
(40.5 ± 0.6 pc)
Absolute magnitude (MV)+1.76
Details
Aa
Mass1.95 M
Radius1.93 R
Luminosity17.44 L
Surface gravity (log g)4.40±0.14 cgs
Temperature9,099±309 K
Metallicity [Fe/H]−0.06 dex
Rotational velocity (v sin i)167.6±1.7 or 13.4±1.5 km/s
Age212 or 30 Myr
Other designations
s Eri, CD−43°814, FK5 2185, HD 16754, HIP 12413, HR 789, SAO 215996
Database references
SIMBADdata

This object was flagged as an astrometric binary based on proper motion measurements made from the Hipparcos spacecraft. Zuckerman et al. (2011) consider it a multi-star system, with a bright A-type primary plus a faint M-type companion at an angular separation of 25 to the north. The astrometric companion to the primary remains unresolved.

The main component is an A-type main-sequence star with a stellar classification of A1 Vb. Based upon stellar models, it has an age estimated at 212 million years. Consistency with its membership in the Columba association suggests a much younger age of 30 million years. Earlier measurements showed a high projected rotational velocity of 168 km/s. However, Ammler-von Eiff and Reiners (2012) found a much lower velocity of 13 km/s.

The visible companion is a red dwarf star with a class in the range M2-5V. The system is a source of X-ray emission with a luminosity of 924×1020 W, which is most likely coming from this component and the unresolved companion.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.