NGC 346

Source: Wikipedia, the free encyclopedia.
Distance
210,000 light-years
Physical characteristics
H II region
Other designationsESO 51-10,[2] N66
Associations
ConstellationTucana[3]
See also: Open cluster, List of open clusters

NGC 346 is a young

multiple star system HD 5980,[6]
one of the brightest stars in the SMC.

This cluster is located near the center of the brightest

earlier.[8] The inner 15 pc radius of the cluster appears centrally condensed, while the area outside that volume is more dispersed.[9] The youngest cluster members near the center have ages of less than two million years,[7] and observations suggests the cluster is still engaged in high mass star formation.[7] The cluster star formation rate is estimated at (4±1)×10−3 M yr−1.[9]

Recent observations[10] by NASA's James Webb Space Telescope have provided unprecedented insights into NGC 346. These observations have revealed surprising details about the cluster's dust environment, challenging previous assumptions and shedding light on the processes of protostar formation and early planetary development within this dynamic stellar nursery. Webb's observations mark a significant advancement in our understanding of star formation in the Small Magellanic Cloud and offer exciting avenues for further research into the cosmic evolution of galaxies.

  • Image of NGC 346 with a 30 arcminute wide field of view showing the wispy nebular structure around it.
    Image of NGC 346 with a 30 arcminute wide field of view showing the wispy nebular structure around it.
Prominent stars[11]
Walborn ELS MPG NMC SSN Spectral
type
Effective
temperature (K)
Absolute
magnitude
Bolometric
magnitude
Mass
(M)
207758 755
(HD 5980/AB5)
LBV
WN4
OI
45,000
45,000
34,000
−7.1
(−8.1) −6.8
−6.7
−11.135
−10.885
−9.885
61
66
34
1 435 26 7 O5.5If 43,400 −6.7 −10.7 91
1 789 5 O7If 38,900 −7 −10.7 85
3 355 29 9 O3V 51,300 −5.7 −10.3 76
6 7 324 32 13 O4V 48,600 −5.2 −9.6 54
4 342 30 11 O5.5V 44,900 −5.5 −9.7 53
368 28 15 O5.5V 44,900 −5 −9.2 43
2 470 25 O8.5III 35,700 −5.4 −8.9 34

See also

References

External links