NGC 2626
Appearance
Reflection nebula | |
---|---|
![]() Atlas Image mosaic of NGC 2626, which, at a distance of about 1 kpc (3300 light years), is primarily reflecting the light from the bright blue (B1-type) 10th-magnitude star, CD-40° 4432, which is embedded in it. | |
Observation data:J2000epoch | |
Right ascension | 08h35m32s[1] |
Declination | −40° 40′ 18″[1] |
Distance | 3900 ± 1110ly(1200 ± 340[2]pc) |
Apparent dimensions (V) | 5.0′× 5.0′[3] |
Constellation | Vela |
Designations | NGC2626, Ced 106h, GN 08.33.7, VdBH 17 |
NGC 2626is areflection nebula,emission nebula,andabsorption nebulain the constellationVela.[4][5]It is mostly illuminated by B1 starCD-40 4432and ionized by the O8 quadruple star systemHD 73882,together with other stars.
Gallery
[edit]-
This image has been produced using observations made at the SMARTS 0.9-meter Telescope at theCerro Tololo Inter-American Observatory(CTIO)[6]
See also
[edit]References
[edit]- ^ab"NGC 2626".SIMBAD.Centre de données astronomiques de Strasbourg.Retrieved11 August2017.
- ^Pinheiro, M. C.; Copetti, M. V. F.; Oliveira, V. A. (2010)."Spectral classification and distance determination of stars in nine southern Galactic H II regions".Astronomy and Astrophysics.521:A26.Bibcode:2010A&A...521A..26P.doi:10.1051/0004-6361/200912937.
- ^Seligman, Courtney."New General Catalogue objects: NGC 2600 - 2649".cseligman.com.Retrieved11 August2017.
- ^Mueller, Kaisa; Graham, John A (November 2000). "Young Stars Associated with the Reflection Nebula NGC 2626".Publications of the Astronomical Society of the Pacific.112(777): 1426–32.Bibcode:2000PASP..112.1426M.doi:10.1086/317705.JSTOR10.1086/317705.S2CID121268925.
- ^Harvey, J.; Mazlin, S.; Verschatse, D.; Perez, J. J. (September 2014). "Rarely Imaged".Astronomy:89.
- ^"A Vista of NGC 2626 with the SMARTS 0.9-meter Telescope".RetrievedApril 20,2021.
External links
[edit]Media related toNGC 2626at Wikimedia Commons