Astronomy:NGC 4361
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Short description: Planetary nebula in the constellation Corvus
| Emission nebula | |
|---|---|
| Planetary nebula | |
| File:300px NGC 4361 imaged with a 24-inch telescope | |
| Observation data: J2000 epoch | |
| Right ascension | 12h 24m 30.8s[1] |
| Declination | −18° 47′ 5.6″[1] |
| Distance | 3,377.2±153.6[1] ly |
| Apparent magnitude (V) | 10.9[2] |
| Apparent dimensions (V) | 1.3' x 1.3'[2] |
| Constellation | Corvus[3] |
| Designations | NGC 4361, PN G294.1+43.6 |
NGC 4361 (also known as the Lawn Sprinkler Nebula[4] or Garden Sprinkler Nebula) is a planetary nebula in the Corvus constellation.[3][1][2] It is included in the Astronomical League's Herschel 400 Observing Program.
Central star
NGC 4361's central star, which has the Henry Draper Catalogue designation HD 107969,[5] is an extremely hot [WC] Wolf-Rayet type star. Its temperature is 126,000 K.[6] It is nearly 18,000 times brighter than the Sun, but is only 6.1% its size. This star left the asymptotic giant branch between 5,776 and 8,018 years ago.[6]
Gallery
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NGC 4361 with legacy surveys
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NGC 4361 imaged in infrared by the Spitzer Space Telescope
References
- ↑ 1.0 1.1 1.2 1.3 "NGC 4361 -- Planetary Nebula". Universite de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-id?mescat.distance=on&mescat.velocities=on&Ident=%401946508&Name=NGC++4361&submit=display+selected+measurements#lab_meas.
- ↑ 2.0 2.1 2.2 "Planetary Nebula NGC 4361". https://telescopius.com/deep-sky/object/5403/ngc-4361/planetary-nebula.
- ↑ 3.0 3.1 Stefan Rumistrzewicz (1 November 2010). A Visual Astronomer's Photographic Guide to the Deep Sky: A Pocket Field Guide. Springer Science & Business Media. pp. 158–. ISBN 978-1-4419-7242-2. https://books.google.com/books?id=Vhjn3DEJpyIC&pg=PA158.
- ↑ Stoyan, Ronald; Schurig, Stephan (2014). interstellarum Deep Sky Atlas. Erlangen: Cambridge University Press; Oculum-Verlag GmbH. ISBN 978-1-107-50338-0. OCLC 920437579. http://www.deep-sky-atlas.com/.
- ↑ Jordan, S.; Bagnulo, S.; Werner, K.; O’Toole, S. J. (2012). "Magnetic fields in central stars of planetary nebulae?". Astronomy & Astrophysics 542: A64. doi:10.1051/0004-6361/201219175. ISSN 0004-6361.
- ↑ 6.0 6.1 González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C. (2019-10-01). "Properties of central stars of planetary nebulae with distances in Gaia DR2" (in en). Astronomy & Astrophysics 630: A150. doi:10.1051/0004-6361/201936162. ISSN 0004-6361. Bibcode: 2019A&A...630A.150G. https://www.aanda.org/articles/aa/abs/2019/10/aa36162-19/aa36162-19.html.
External links
