Jump to content

HD 65750

From Wikipedia, the free encyclopedia
HD 65750

The nebula surrounding HD 65750
Observation data
Epoch J2000      Equinox J2000
Constellation Carina
Right ascension 07h 56m 50.94795s[1]
Declination −59° 07′ 32.7605″[1]
Apparent magnitude (V) 6.2 - 7.1[2]
Characteristics
Spectral type M1 II[3]
U−B color index +2.18[4]
B−V color index +1.93[4]
Variable type LB[5]
Astrometry
Radial velocity (Rv)23.17 km/s
Proper motion (μ) RA: -4.030[6] mas/yr
Dec.: 9.789[6] mas/yr
Parallax (π)2.6230 ± 0.0931 mas[6]
Distance1,240 ± 40 ly
(380 ± 10 pc)
Details
Mass1.11[7] M☉
Radius103[6] R☉
Luminosity1,698[6] L☉
Surface gravity (log g)0.31[7] cgs
Temperature3,650[6] K
Metallicity [Fe/H]-0.4[8] dex
Other designations
V341 Car, CD-58°1926, HD 65750, HIP 38834, SAO 235638, HR 3126[9]
Database references
SIMBADdata

HD 65750, also known as V341 Carinae is a bright red giant star in the constellation Carina. It is surrounded by a prominent reflection nebula,[10][9] known as IC 2220, nicknamed the Toby Jug Nebula.

Characteristics

[edit]
A light curve for V341 Carinae, plotted from Hipparcos data.[11]

HD 65750 is located about 900 light years away, and has an apparent magnitude that varies between 6.2 and 7.1 and a metallicity just 40% of the Sun. It is part of the Diamond Cluster moving group.

The star has a radial velocity of 20 km/s.[12] The star has a radius over 100 times wider than the Sun's; were it to replace the Sun, HD 65750 would extend past the orbit of Mercury.

Nebulae

[edit]

The nebulae is a mystery as the variations in nebulae brightness appear to be unrelated to the host star.[13] One theory is that rather than being an accreting protoplanetary disk the star may be an evolved star that is losing material.[14][15]

References

[edit]
  1. ^ a b van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
  2. ^ "V341 Carinae". International Variable Star Index. AAVSO. Retrieved 2020-03-04.
  3. ^ Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins Catalog of Revised MK Types for the Cooler Stars". The Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
  4. ^ a b Dachs, J. (2000). "On the photometric variations of the red giant HD 65750 and of the surrounding reflection nebula IC 2220". Astronomy and Astrophysics. 63 (3): 353–362. Bibcode:1978A&A....63..353D.
  5. ^ Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1: B/gcvs. Bibcode:2009yCat....102025S.
  6. ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  7. ^ a b Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy and Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. S2CID 131780028.
  8. ^ Castilho, B. V. (2000). "Detailed analysis of a sample of Li-rich giants". Astronomy and Astrophysics. 364: 674–682. Bibcode:2000A&A...364..674C.
  9. ^ a b "HD 65750". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-03-04.
  10. ^ "HIP 38834". Archived from the original on 2015-09-26. Retrieved 2019-06-28.
  11. ^ "Hipparcos Tools Interactive Data Access". Hipparcos. ESA. Retrieved 8 December 2021.
  12. ^ "IC 2220 - The Toby Jug Nebula". Retrieved 2019-06-28.
  13. ^ Dachs, J.; Isserstedt, J.; Rahe, J. (1978). "On the photometric variations of the red giant HD 65750 and of the surrounding reflection nebula IC 2220". Astronomy and Astrophysics. 63: 353. Bibcode:1978A&A....63..353D.
  14. ^ Humphreys, R. M.; Ney, E. P. (1974). "Infrared observations of HD 65750, a red giant in a reflection nebula". Astronomy and Astrophysics. 30: 159. Bibcode:1974A&A....30..159H.
  15. ^ ESO, Garching, Germany (October 14, 2013). "A close look at the Toby Jug Nebula". Astronomy magazine. Retrieved 2019-06-28.{{cite web}}: CS1 maint: multiple names: authors list (link)
Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_65750&oldid=1256433321"