LSS 4067

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LSS 4067
Observation data
J2000
Constellation
Scorpius
Right ascension 17h 19m 05.548s[1]
Declination −29° 43′ 41.1989″[1]
Apparent magnitude (V) 11.44[2]
Characteristics
Spectral type O4.5Ifpe[3]
U−B color index +0.37[2]
B−V color index +1.49[2]
V−R color index +1.28[2]
Distance
9,500–12,700 ly
(2,900–3,900[2] pc)
Absolute magnitude (MV)−6.335[6]
Details
Myr
CD−38°11748, Hen 3-1374, HM 1 VB 4, TYC 7870-896-1, 2MASS
J17190554-3848496
Database references
SIMBADdata

LSS 4067, also known as CD−38°11748, is an

interstellar extinction, so its apparent magnitude is brighter for longer-wavelength passbands.[2] Without the extinction, it is estimated that LS 4067 would be 5.8 magnitudes brighter, a naked eye star with an apparent magnitude of 5.3.[9]

Although the

Gaia Data Release 2 parallax for LS 4067 is negative, a likely distance can be calculated from it. The star is thought to be between 8,202 and 14,084 pc away, statistically most likely at 10,170 pc.[10] It was catalogued as a member of the faint cluster Havlen-Moffat No. 1, but is no longer thought to be a member. The cluster lies about 3,300 pc.[2]

LSS 4067 has an

spectral type.[4] Because of this unusual spectrum, classifying the star or deducing its properties has proved relatively difficult: for example, the effective temperature is predicted to be too cool and the surface gravity too high.[4]

See also

References