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LH41-1042

LH41-1042
Eso9931d.jpg
The N119 Hii region. LH41-1042 and LMC195-1 are both in the central core of the dense cluster to the right of centre.
Credit: ESO
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Dorado
Right ascension +05h 18m 11.01s
Declination −69° 13′ 11.3″
Apparent magnitude (V) 13.95
Characteristics
Spectral type WO4
U−B color index −1.38
B−V color index +0.31
Astrometry
Distance 160,000 ly
(49,000 pc)
Details
Mass 8.4 M
Radius 0.62 R
Luminosity 182,000 L
Temperature 150,000 K
Other designations
LH 41-1042
Database references
SIMBAD data

LH41-1042 is a Wolf-Rayet star located in the Large Magellanic Cloud (LMC). It is an extremely rare member of the WO oxygen sequence, the second to be discovered in the LMC and one of only three found so far.

The star was identified in 2012 during an investigation of the LH41 stellar association, also known as NGC 1910, using one of the 6.5m Magellan Telescopes at Las Campanas Observatory in Chile.

LH 41-1042 is located in the rich LH 41 (NGC 1910) stellar association that contains two luminous blue variables, S Doradus and R85, the WN5 star BAT99-27, and another WO star LMC195-1. The two WO stars are only 9" apart. WO stars are classified on the basis of OVI emission at 381.1-383.4 nm, which is weak or absent in other Wolf Rayet stars. The WO4 subclass is defined as having the ratio of OVI to OV emission strength between 0.5 and 1.8. In the new star, the ratio of these line strengths was 0.7.

The high temperature and high luminosity of LH 41-1042 produce a stellar wind travelling at 3,500 km/s and it is losing mass about a billion times more quickly than the sun. It is estimated that it has exhausted its core helium and only has 9,000 years left before it explodes as a type Ic supernova.


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