狐狸座OB1

狐狸座OB1
狐狸座OB1
	狐狸座OB1
觀測數據
星座	狐狸座
赤經	19h 44.0m
赤緯	+24° 13′
平均距離	5.2 kly（1.6 kpc）
徑向速度	3.1 km/s
物理性質
其它名稱	Vul OB1
	相關條目:星協、移動星群

狐狸座OB1是一個在其中誕生了一批大質量恆星的OB星協。它最早是由W.W.摩根（1953年）等人確認的^[4]。該星協位於獵戶臂，距離太陽大約7,500光年^[5]。包含在這個星協中的星雲包括NGC 6820和NGC 6823^[4]，以及 Sh2-88^[5]。

狐狸座OB1包含近100顆OB型恆星和800多顆年輕恆星天體。該星協長約100秒差距，且均勻形成。這個年輕恆星天體以兩個群體的形式存在，一個群體代表孤立的年輕恆星天體，另一個群體包括紅外星雲。在Sh2-86、Sh 2-87、Sh 1-88、緻密HII區和其它星團，例如Cr 404周圍，都有很多年輕恆星天體的族群。這被懷疑是由觸發的恆星形成引起的。OB型恆星在這個區域塑造了許多柱狀結構^[6]。

參考資料

^ ^1.0 ^1.1 ^1.2 Vul OB1. SIMBAD. 斯特拉斯堡天文資料中心.
^ Melnik, A. M.; Dambis, A. K. Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions. Astrophysics and Space Science. 2020, 365 (7): 112. Bibcode:2020Ap&SS.365..112M. S2CID 220128144. arXiv:2006.14649 . doi:10.1007/s10509-020-03827-0.
^ Mel'Nik, A. M.; Dambis, A. K. Kinematics of OB-associations and the new reduction of the Hipparcos data. Monthly Notices of the Royal Astronomical Society. 2009, 400 (1): 518. Bibcode:2009MNRAS.400..518M. arXiv:0909.0618 . doi:10.1111/j.1365-2966.2009.15484.x .
^ ^4.0 ^4.1 Thé, P. S.; van Paradijs, J. A. UBV photoelectric photometry of early type stars in the direction of the associations Vul OB 1 and Vul OB 4.. Astronomy and Astrophysics. July 1971, 13: 274. Bibcode:1971A&A....13..274T.
^ ^5.0 ^5.1 Billot, N.; et al. Young Stellar Objects and Triggered Star Formation in The Vulpecula OB Association. The Astrophysical Journal. April 2010, 712 (2): 797–812. Bibcode:2010ApJ...712..797B. S2CID 28961682. arXiv:1003.0866 . doi:10.1088/0004-637X/712/2/797.
^ Billot, N.; Noriega-Crespo, A.; Carey, S.; Guieu, S.; Shenoy, S.; Paladini, R.; Latter, W. Young Stellar Objects and Triggered Star Formation in The Vulpecula OB Association. The Astrophysical Journal. 2010-04-01, 712 (2): 797–812 [2024-02-25]. Bibcode:2010ApJ...712..797B. ISSN 0004-637X. S2CID 28961682. arXiv:1003.0866 . doi:10.1088/0004-637X/712/2/797. （原始內容存檔於2022-12-26）.

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[SIMBAD-1] 1.0 ^1.1 ^1.2 Vul OB1. SIMBAD. 斯特拉斯堡天文資料中心.

[melnik-2] Melnik, A. M.; Dambis, A. K. Distance scale for high-luminosity stars in OB associations and in field with Gaia DR2. Spurious systematic motions. Astrophysics and Space Science. 2020, 365 (7): 112. Bibcode:2020Ap&SS.365..112M. S2CID 220128144. arXiv:2006.14649 . doi:10.1007/s10509-020-03827-0.

[MelNik2009-3] Mel'Nik, A. M.; Dambis, A. K. Kinematics of OB-associations and the new reduction of the Hipparcos data. Monthly Notices of the Royal Astronomical Society. 2009, 400 (1): 518. Bibcode:2009MNRAS.400..518M. arXiv:0909.0618 . doi:10.1111/j.1365-2966.2009.15484.x .

[Thé1971-4] 4.0 ^4.1 Thé, P. S.; van Paradijs, J. A. UBV photoelectric photometry of early type stars in the direction of the associations Vul OB 1 and Vul OB 4.. Astronomy and Astrophysics. July 1971, 13: 274. Bibcode:1971A&A....13..274T.

[Billot2010-5] 5.0 ^5.1 Billot, N.; et al. Young Stellar Objects and Triggered Star Formation in The Vulpecula OB Association. The Astrophysical Journal. April 2010, 712 (2): 797–812. Bibcode:2010ApJ...712..797B. S2CID 28961682. arXiv:1003.0866 . doi:10.1088/0004-637X/712/2/797.

[6] Billot, N.; Noriega-Crespo, A.; Carey, S.; Guieu, S.; Shenoy, S.; Paladini, R.; Latter, W. Young Stellar Objects and Triggered Star Formation in The Vulpecula OB Association. The Astrophysical Journal. 2010-04-01, 712 (2): 797–812 [2024-02-25]. Bibcode:2010ApJ...712..797B. ISSN 0004-637X. S2CID 28961682. arXiv:1003.0866 . doi:10.1088/0004-637X/712/2/797. （原始內容存檔於2022-12-26）.

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