NGC 6357
| سديم انبعاثي | |
|---|---|
| H II region | |
 | |
| بيانات الرصد: حقبة J2000 | |
| الصعود المستقيم | 17h 24m[1] |
| الميل | −34° 20′[1] |
| المسافة | ~ 8000[2] س.ض. |
| الكوكبة | العقرب[3] |
| تسميات | War and Peace Nebula,[1] Lobster Nebula [4] Sharpless 11, RCW 131, Gum 66 |
NGC 6357 هي سديم انتشاري بالقرب من NGC 6334 في كوكبة العقرب. ويضم السديم العديد من النجوم الأولية تحميها أقراص داكنة من الغاز، نجوم حديثة مغلفة في "شرانق" تتمدد أو غازات متمددة تحيط بتلك النجوم الصغيرة. وتُعرف أيضاً بإسم سديم السلطعون Lobster Nebula[4][5]
وهذا السديم قد أُطلِق عليه أيضاً اسم سديم الحرب والسلام من قِبل علماء تجربة فضاء منتصف الطريقMidcourse Space Experiment بسبب مظهرها. They said that in infrared images the bright, western part resembles a dove, while the eastern part looks like a skull.[6]
NGC 6357 and Pismis 24
Pismis 24
This nebula includes the open cluster Pismis 24, which is home to several massive stars. One of the brightest stars in the cluster, Pismis 24-1, was thought possibly to be the most massive on record, approaching 300 solar masses, until it was discovered to be a multiple system of at least three stars; component stars would still remain near 100 solar masses, making them among the more massive stars on record.[7][8]
| Star (Pismis 24-#) |
Spectral type | Magnitude (Mbol) |
Temperature[10] (K) |
Radius (R☉) |
Mass (M☉) |
|---|---|---|---|---|---|
| 1NE | O3.5 If* | −10.0 | 42,000 | 17 | 74 |
| 1SW | O4 III | −9.8 | 41,500 | 16 | 66 |
| 2 | O5.5 V(f) | −8.9 | 40,000 | 12 | 43 |
| 3 | O8 V | −7.7 | 33,400 | 9 | 25 |
| 10 | O9 V | −7.2 | 31,500 | 8 | 20 |
| 12 | B1 V | −5.3 | 30,000 | 4 | 11 |
| 13 | O6.5 III((f)) | −8.6 | 35,600 | 12 | 35 |
| 15 | O8 V | −7.8 | 33,400 | 10 | 25 |
| 16 | O7.5 V | −9.0 | 34,000 | 16 | 38 |
| 17 | O3.5 III | −10.1 | 42,700 | 17 | 78 |
| 18 | B0.5 V | −6.4 | 30,000 | 6 | 15 |
| 19 | B0.5 V | −5.4 | 30,000 | 4 | 11 |
G353.2+0.7
The young stellar cluster G353.2+0.7 lies east of Pismis 24 and was revealed by a Chandra X-ray image showing approximately 800 stars.[11]
G353.1+0.36
The young stellar cluster G353.1+0.36 lies southeast of Pismis 24 and also contains approximately 800 stars detected by X-ray.[11] The region includes several O-type stars, including [BDSB2003] 10.[12]
الهامش
- ^ أ ب ت "SIMBAD Astronomical Database". Results for NGC 6357. Retrieved 2007-05-03.
- ^ Robert Nemiroff; Jerry Bonnell (21 November 2010). "A Massive Star in NGC 6357". Astronomy Picture of the Day.
- ^ R. W. Sinnott, ed. (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 0-933-34651-4.
- ^ أ ب http://www.theguardian.com/science/2013/feb/20/lobster-nebula-birthplace-stars-infrared
- ^ http://www.space.com/19938-lobster-nebula-seen-with-esos-vista-telescope-space-wallpaper.html
- ^ "2MASS Picture of the Week Archive Captions".
- ^ "ESA Science & Technology: Star on a Hubble diet NGC 6357". Retrieved 2007-04-11.
- ^ NASA: Massive Stars in Open Cluster Pismis 24, 2006
- ^ DOI:10.1051/0004-6361/201015914
This citation will be automatically completed in the next few minutes. You can jump the queue or expand by hand - ^ DOI:10.1051/0004-6361:20042386
This citation will be automatically completed in the next few minutes. You can jump the queue or expand by hand - ^ أ ب Townsley, L. K.; et al. (2014). "The Massive Star-Forming Regions Omnibus X-Ray Catalog". Astrophysical Journal Supplement. 213 (1): 1. arXiv:1403.2576. Bibcode:2014ApJS..213....1T. doi:10.1088/0067-0049/213/1/1.
- ^ Damke, G.; et al. (2006). "The open cluster G353.1+0.7 in NGC6357". Revista Mexicana de Astronomía y Astrofísica. 26: 180. Bibcode:2006RMxAC..26..180D.
وصلات خارجية
- A Massive Star in NGC 6357 with a close-up of Pismis 24.
- Star Forming Region NGC 6357 showing complex interactions between interstellar winds, radiation pressures and magnetic fields.
- NGC 6357: Massive Stars
- A Massive Star in NGC 6357