CPD−57°2874

Star in the constellation Carina From Wikipedia, the free encyclopedia

CPD−57°2874 is a B[e] supergiant in the constellation Carina.[8] It is a rare star as it is hot but has dust which shows forbidden lines and IR emissions.[9] In 2007 the high spatial and spectral resolution of the star's circumstellar envelope was studied. This was the first time such a study was carried out on a class B[e] supergiant.[6][10]

Right ascension10h 15m 21.9711s[2]
Declination−57° 51 42.713[2]
Quick facts Constellation, Right ascension ...
CPD−57°2874
Observation data
Epoch J2000      Equinox ICRS
Constellation Carina[1]
Right ascension 10h 15m 21.9711s[2]
Declination −57° 51 42.713[2]
Apparent magnitude (V) +10.08[3]
Characteristics
Spectral type sgB1[e][3][4]
U−B color index +0.30[3]
B−V color index +1.65[3]
Variable type suspected[4][5]
Astrometry
Radial velocity (Rv)−54[6] km/s
Proper motion (μ) RA: −5.90[2] mas/yr
Dec.: 5.10[2] mas/yr
Distance3,440[6] pc
Absolute magnitude (MV)−7.7[6]
Details
Mass17.4–18.6[6] M
Radius60[3] R
Luminosity500,000[7] L
Temperature20,000[3] K
Rotational velocity (v sin i)36 ± 4[6] km/s
Other designations
CD−57°3107, CPD−57°2874, GSC 08608-00427, PPM 769178
Database references
SIMBADdata
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Disc

CPD−57°2874 is surrounded by a disc of expelled stellar material. The inner edge of the disc is 27.5 AU from the star and it is inclined at an angle of 46° to us. The particular alignment, temperature, and density of the disc combine to produce the forbidden spectral lines. The detached ring leads to speculation that the inner regions are cleared by an unseen binary companion.[6]

Variability

Photometry of CPD−57°2874 suggests that its brightness is variable with an amplitude of perhaps 0.2 magnitude. It has not been formally classified as a variable star and the cause of the variations is unclear.[6]

See also

References

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