A faint blue galaxy (FBG) is an inconspicuous, often small galaxy with low surface luminosity. In addition to being dim, they show a remarkable preponderance of sparsely scattered blue stars, but comparatively few red stars, which in most galaxies are by far the most common. They appear as dim, bluish smudges on old photographic plates, with no clear structure or shape, and do not register well on modern electronic cameras, which are more sensitive to red light. They are currently interpreted as small dwarf-irregular satellite-galaxies undergoing a burst of star formation.[1]
YouTube Encyclopedic
-
1/3Views:482 025432 92565 449
-
Galaxies, part 1: Crash Course Astronomy #38
-
Galaxies, part 2: Crash Course Astronomy #39
-
Universe Documentary 2017 | White Dwarf - Universe's Sleeping Monster | National Geographic
Transcription
Previously overlooked
Although some had been previously photographed as faint smudges in sky surveys, they were first noticed in the 1970s, posing a problem for then-current theories of galaxy formation. FBGs tend to found in the peripheries of galaxy clusters and as remote satellites of large galaxies, and appear to be a now-finished stage of galactic growth.[2][3] Any galaxy might appear faint because it is small or because it is far away. Neither explanation, nor any combination, matched the initial FBG observations.
The first faint blue galaxy problem
The faint blue galaxy (FBG) problem in astrophysics first arose with observations starting in 1978 that there were more galaxies with a bolometric magnitude > 22 than then-current theory predicted.[4][5][6]
The distribution of these galaxies has since been found to be consistent with models of cosmic inflation, measurements of the cosmic microwave background, and a nonzero cosmological constant; that is, with the existence of the now-accepted dark energy.[7][8] It thus serves as a confirmation of supernova observations requiring dark energy.
The second faint blue galaxy problem
A second problem arose in 1988, with even deeper observations showing a much greater excess of faint galaxies.[9]
These are now interpreted as dwarf galaxies experiencing large bursts of stellar formation, resulting in blue light from young, massive stars.[1] Thus FBGs are extremely bright for their size and distance.
Most FBGs appear between red-shift z = 0.5–2. It is inferred that they merged with other galaxies and consequently disappeared as separate objects some time in the "recent" cosmological past.[2][3]
References
- ^ a b Colless, Matthew; Ellis, Richard S.; Broadhurst, T. J.; Taylor, Keith; Peterson, Bruce A. (March 1993). "Faint blue galaxies – High or low redshift?". Monthly Notices of the Royal Astronomical Society. 261: 19–38. Bibcode:1993MNRAS.261...19C. doi:10.1093/mnras/261.1.19. hdl:1885/39978.
- ^ a b Carlberg, R. G. (November 1992). "Merging and fast galaxy evolution". Astrophysical Journal Letters. 399 (1): L31–L34. Bibcode:1992ApJ...399L..31C. doi:10.1086/186599.
- ^ a b Carlberg, R. G.; Charlot, Stephane (September 1992). "Faint galaxy evolution via interactions". Astrophysical Journal. 397 (1): 5–13. Bibcode:1992ApJ...397....5C. doi:10.1086/171759.
- ^ Kron, Robert G. (1978). Photometry of a Complete Sample of Faint Galaxies (Ph.D. thesis). Berkeley, California: University of California. Bibcode:1978PhDT........13K.
- ^ Peterson, B. A.; Ellis, R. S.; Kibblewhite, E. J.; Bridgeland, M. T.; Hooley, T.; Horne, D. (1 November 1979). "Number magnitude counts of faint galaxies". Astrophysical Journal Letters. 233: L109–L113. Bibcode:1979ApJ...233L.109P. doi:10.1086/183087.
- ^ Tyson, J. A.; Jarvis, J. F. (15 June 1979). "Evolution of galaxies – Automated faint object counts to 24th magnitude". Astrophysical Journal Letters. 230: L153–L156. Bibcode:1979ApJ...230L.153T. doi:10.1086/182982.
- ^ Yoshii, Yuzuru; Takahara, Fumio (1 November 1989). "On the redshift-volume measurement of the cosmological density parameter". Astrophysical Journal. 346: 28–33. Bibcode:1989ApJ...346...28Y. doi:10.1086/167983.
- ^ David C., Koo (21–23 June 1989). "The evolution of field galaxies – Is Omega = 1?". Evolution of the universe of galaxies; Proceedings of the Edwin Hubble Centennial Symposium. Berkeley, California: Astronomical Society of the Pacific. pp. 268–285. Bibcode:1990ASPC...10..268K.
- ^ Broadhurst, T. J.; Ellis, R. S.; Shanks, T. (1 December 1988). "The Durham/Anglo-Australian Telescope faint galaxy redshift survey". Monthly Notices of the Royal Astronomical Society. 235 (3): 827–856. Bibcode:1988MNRAS.235..827B. doi:10.1093/mnras/235.3.827.
This page was last edited on 22 January 2024, at 04:26