NGC 1501

NGC 1501
發射星雲
行星狀星雲
	從哈伯太空望遠鏡看到的NGC 1501
觀測資料: J2000 epoch
赤經	04h 06m 59.39s
赤緯	+60° 55′ 14.4″
距離	est. 4,240 ly（1.30 kpc）光年
視星等 (V)	13.0
視尺度(V)	0.863' (diameter)
星座	鹿豹座
物理性質
半徑	0.5 ly
名稱	PK 144+6.1、PN G 144.5+06.5、GC 801、CS 14.4、H 4.53
	相關條目：星雲列表

NGC 1501是一個複雜的行星狀星雲，威廉·赫歇爾於1787年8月27日在鹿豹座這個星座內發現它^[2]^[3]。它也被稱為牡蠣星雲^[4]。

性質

行星狀星雲的中心恆星的光譜類型為[WC4]，類似於富含碳的沃夫–瑞葉星^[5]。它是一顆脈動的恆星，這意味着它的亮度有規律地和週期性地變化。就NGC 1501的前身恆星而言，這是非常快的，恆星的亮度在短短半小時內發生了顯著變化。分析蓋亞的數據表明，中央恆星是一個聯星系統^[6]。可見光觀測捕捉到包括氫氣和氮氣在內的氣體輝光^[7]。星雲的總質量估計約為0.22 M_☉，其中大部分是電離氣體（0.21 M_☉）和一小部分（6996890000000000000♠8.9×10⁻⁴ M_☉）是富含碳的灰塵^[8]。

圖集

NGC 1501的位置（用紅圈標出）
使用萊蒙山天空中心的0.8m舒爾曼望遠鏡拍攝的NGC 1501

參考資料

^ ^1.0 ^1.1 ^1.2 SIMBAD Astronomical Database. NGC 1501. [2014-11-09]. （原始內容存檔於2014-11-10）.
^ ^2.0 ^2.1 Sabbadin, F.; Benetti, S.; Cappellaro, E.; Turatto, M. The tetra-lobed planetary nebula NGC 1501. Astronomy and Astrophysics. 2000, 361: 1112–1120. Bibcode:2000A&A...361.1112S. arXiv:astro-ph/0007039 .
^ Seligman, Courtney. Celestial Atlas: NGC Objects: NGC 1500 - 1549. cseligman.com. [10 July 2015]. （原始內容存檔於1 January 2016）.
^ Hubble View of Bubbly Nebula. 17 April 2015 [8 December 2016]. （原始內容存檔於2016-09-18）.
^ González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C.; López Varela, P. Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity. Astronomy & Astrophysics. 2021, 656: A51. Bibcode:2021A&A...656A..51G. S2CID 237940344. arXiv:2109.12114 . doi:10.1051/0004-6361/202141916.
^ Chornay, N.; Walton, N. A.; Jones, D.; Boffin, H. M. J.; Rejkuba, M.; Wesson, R. Towards a more complete sample of binary central stars of planetary nebulae with Gaia. Astronomy & Astrophysics. 2021, 648: A95. Bibcode:2021A&A...648A..95C. S2CID 230770301. arXiv:2101.01800 . doi:10.1051/0004-6361/202140288.
^ Oyster Nebula NGC 1501 As Seen By Hubble - SpaceRef. spaceref.com. 7 September 2016 [2021-02-08]. ^{[失效連結]}
^ Rubio, G.; Toalá, J. A.; Todt, H.; Sabin, L.; Santamaría, E.; Ramos-Larios, G.; Guerrero, M. A. Planetary nebulae with Wolf–Rayet-type central stars – IV. NGC 1501 and its mixing layer. Monthly Notices of the Royal Astronomical Society. 2022, 517 (4): 5166–5179. Bibcode:2022MNRAS.517.5166R. arXiv:2210.09116 . doi:10.1093/mnras/stac3011.

外部連結

維基共享資源上的相關多媒體資源：NGC 1501
http://www.astronomy-mall.com/Adventures.In.Deep.Space/abellcat^{[永久失效連結]}
http://www.observing.skyhound.com/archives/dec/NGC_1501^{[失效連結]}

[simbad-1] 1.0 ^1.1 ^1.2 SIMBAD Astronomical Database. NGC 1501. [2014-11-09]. （原始內容存檔於2014-11-10）.

[sabbadin2000-2] 2.0 ^2.1 Sabbadin, F.; Benetti, S.; Cappellaro, E.; Turatto, M. The tetra-lobed planetary nebula NGC 1501. Astronomy and Astrophysics. 2000, 361: 1112–1120. Bibcode:2000A&A...361.1112S. arXiv:astro-ph/0007039 .

[Seligman-3] Seligman, Courtney. Celestial Atlas: NGC Objects: NGC 1500 - 1549. cseligman.com. [10 July 2015]. （原始內容存檔於1 January 2016）.

[Hubble-4] Hubble View of Bubbly Nebula. 17 April 2015 [8 December 2016]. （原始內容存檔於2016-09-18）.

[5] González-Santamaría, I.; Manteiga, M.; Manchado, A.; Ulla, A.; Dafonte, C.; López Varela, P. Planetary nebulae in Gaia EDR3: Central star identification, properties, and binarity. Astronomy & Astrophysics. 2021, 656: A51. Bibcode:2021A&A...656A..51G. S2CID 237940344. arXiv:2109.12114 . doi:10.1051/0004-6361/202141916.

[Chornay-6] Chornay, N.; Walton, N. A.; Jones, D.; Boffin, H. M. J.; Rejkuba, M.; Wesson, R. Towards a more complete sample of binary central stars of planetary nebulae with Gaia. Astronomy & Astrophysics. 2021, 648: A95. Bibcode:2021A&A...648A..95C. S2CID 230770301. arXiv:2101.01800 . doi:10.1051/0004-6361/202140288.

[hubb-7] Oyster Nebula NGC 1501 As Seen By Hubble - SpaceRef. spaceref.com. 7 September 2016 [2021-02-08]. ^{[失效連結]}

[Rubio-8] Rubio, G.; Toalá, J. A.; Todt, H.; Sabin, L.; Santamaría, E.; Ramos-Larios, G.; Guerrero, M. A. Planetary nebulae with Wolf–Rayet-type central stars – IV. NGC 1501 and its mixing layer. Monthly Notices of the Royal Astronomical Society. 2022, 517 (4): 5166–5179. Bibcode:2022MNRAS.517.5166R. arXiv:2210.09116 . doi:10.1093/mnras/stac3011.

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]