Astronomy:G79.29+0.46
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 20h 31m 42.2847s[1] |
| Declination | +40° 21′ 59.0744″[1] |
| Apparent magnitude (V) | 15.1[2] |
| Characteristics | |
| Spectral type | B:I[e][3] |
| Astrometry | |
| Radial velocity (Rv) | 39.02±7.30[1] km/s |
| Proper motion (μ) | RA: −2.925[1] mas/yr Dec.: −5.339[1] mas/yr |
| Parallax (π) | 0.5725 ± 0.0596[1] mas |
| Distance | approx. 5,700 ly (approx. 1,700 pc) |
| Absolute magnitude (MV) | −10[4] |
| Details | |
| Luminosity | 2.51×105[5] L☉ |
| Temperature | 20,400[5] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
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G79.29+0.46 is a luminous blue variable star candidate located in the Cygnus X star formation region.[1][5] In the infrared and at radio wavelengths a prominent circular nebula can be seen. This nebula was formed by past mass-loss episodes of the LBV candidate.[6]
G79.29+0.46 was first reported as a suspected LBV by Higgs, Wendker & Landecker in 1993 with the DRAO Synthesis Telescope, which identified a nebula around a star that was a wind-blown shell.[7] As an LBV candidate, it has a spectrum with many emission lines, H-alpha being the strongest. The spectrum is similar to other LBVs and Be supergiants. The strength of the H-alpha line suggest very dense winds around this star.[3] The star is currently losing mass at a rate of 1.4×10−6 M☉/year and it is surrounded by a dusty envelope with a temperature of 40 to 1,200 K.[5] The star is considered only a candidate LBV because it has not shown variability in the optical or near-infrared over 20 years. It has been suggested that it is a LBV in the quiescent stage.[5]
From radio and infrared images a detached shell can be seen that shows evidence of two mass-loss episodes.[6] This shell has a mass of 1.51 M☉ and a radius of 0.66 parsecs,[5] and it contains carbon monoxide[8] and ammonia.[6]
Gallery
Spitzer and WISE view of G79.29+0.46, the H II-region DR15 (bright object lower left) and the IRDC G79.3+0.3 (dark clouds)[6]
The outer shell is best seen between 20 and 70 Microns, here an image by Spitzer and Herschel.
Radio image of G79.29+0.46 at 1.4 GHz
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 Gaia Collaboration (2022-05-01). "VizieR Online Data Catalog: Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)". VizieR Online Data Catalog: I/355. Bibcode: 2022yCat.1355....0G.
- ↑ Kohoutek, L.; Wehmeyer, R. (1997). "Catalogue of stars in the Northern Milky Way having H-alpha in emission". Astronomische Abhandlungen der Hamburger Sternwarte 11: 1. Bibcode: 1997AAHam..11.....K.
- ↑ 3.0 3.1 Voors, R. H. M.; Geballe, T. R.; Waters, L. B. F. M.; Najarro, F.; Lamers, H. J. G. L. M. (2000-10-01). "Spectroscopy of the candidate luminous blue variable at the center of the ring nebula G79.29+0.46". Astronomy and Astrophysics 362: 236–244. ISSN 0004-6361. Bibcode: 2000A&A...362..236V.
- ↑ Higgs, L. A.; Wendker, H. J.; Landecker, T. L. (1994-11-01). "G 79.29+0.46: a young stellar-wind shell in Cygnus X.". Astronomy and Astrophysics 291: 295–309. ISSN 0004-6361. Bibcode: 1994A&A...291..295H.
- ↑ 5.0 5.1 5.2 5.3 5.4 5.5 Agliozzo, C.; Noriega-Crespo, A.; Umana, G.; Flagey, N.; Buemi, C.; Ingallinera, A.; Trigilio, C.; Leto, P. (2014-05-01). "The candidate luminous blue variable G79.29+0.46: a comprehensive study of its ejecta through a multiwavelength analysis". Monthly Notices of the Royal Astronomical Society 440 (2): 1391–1409. doi:10.1093/mnras/stu296. ISSN 0035-8711. Bibcode: 2014MNRAS.440.1391A.
- ↑ 6.0 6.1 6.2 6.3 Rizzo, J. R.; Palau, Aina; Jiménez-Esteban, F.; Henkel, C. (2014-04-01). "Ammonia observations in the LBV nebula G79.29+0.46. Discovery of a cold ring and some warm spots". Astronomy and Astrophysics 564: A21. doi:10.1051/0004-6361/201323170. ISSN 0004-6361. Bibcode: 2014A&A...564A..21R.
- ↑ Higgs, L. A.; Wendker, H. J.; Landecker, T. L. (1993). "Discovery of a Young Stellar-Wind Shell in Cygnus X". American Astronomical Society Meeting Abstracts 183. Bibcode: 1993AAS...183.5801H.
- ↑ Rizzo, J. R.; Jiménez-Esteban, F. M.; Ortiz, E. (2008-07-01). "Discovery of Warm and Dense Molecular Gas Surrounding the Ring Nebula G79.29+0.46". The Astrophysical Journal 681 (1): 355–364. doi:10.1086/588455. ISSN 0004-637X. Bibcode: 2008ApJ...681..355R.
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