RT Virginis

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RT Virginis

A visual band light curve for RT Virginis, plotted from ASAS data[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 13h 02m 37.981s[2]
Declination +05° 11′ 08.36″[2]
Apparent magnitude (V) 7.7 to 9.7[3]
Characteristics
Evolutionary stage AGB[4]
Spectral type M8III[5]
B−V color index 1.352±0.031[6]
Variable type SRb[7]
Distance
740 ± 20 ly
(226 ± 7 pc)
Absolute magnitude (MV)2.94[6]
Details
dex
PPM 159423[11]
Database references
SIMBADdata

RT Virginis is a

light years.[3] It is receding from the Sun with a radial velocity of 17 km/s.[4]

The long period variability of this star was discovered by

semiregular variable star of the SRb type.[13] The period was determined to be 155 days by P. N. Kholopov and associates in 1985, then re-evaluated as 375 days based on AAVSO light curves in 1997. This is an oxygen-rich red giant star on the asymptotic giant branch of its evolution, and is undergoing mass loss due to thermal pulsation.[9]

Water vapor

emission in the vicinity of the star was detected in the microwave band by D. F. Dickinson in 1973.[14] This is originating from strong maser emission in a circumstellar gas-dust shell.[15] The flux density of these water masers is over 100 Jy.[9] The star is losing mass at a rate of 3×10−6 M·yr−1;[8] the equivalent of the Sun's mass in 3.3 million years. The velocity of the spherically expanding gas is as high as 11 km/s in the water maser region, at a radius of 5 to 25 AU. In a SiO emitting region located ~400 AU from the star, the gas velocity is 7.8 km/s.[16] This outflow appears clumpy and asymmetrical[17] with a strong temporal variation.[15]

References

  1. ^ ASAS All Star Catalogue, The All Sky Automated Survey, retrieved 16 September 2022.
  2. ^ .
  3. ^ , 99.
  4. ^ , A45.
  5. ^ .
  6. ^ .
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  8. ^ .
  9. ^ .
  10. ^ .
  11. ^ "RT Vir", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2022-09-07
  12. .
  13. .
  14. .
  15. ^ .
  16. , A72.
  17. .

Further reading