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'''NGC 1783''' (also known as '''ESO 85-SC29''') is a [[globular cluster]] within the [[Dorado]] constellation and part of the [[Large Magellanic Cloud]], a satellite dwarf galaxy of the [[Milky Way]]. At an aperture of 50 arcseconds, its apparent V-band magnitude is 10.39,<ref name=Song/> making it one of the brightest globular clusters in the LMC as viewed from Earth. It was discovered in 1835 by [[John Herschel]]. The compiler of the [[New General Catalogue]], [[John Louis Emil Dreyer]], described this cluster as "considerably bright, large, round, very gradually pretty much brighter middle, mottled but not resolved."<ref name="cseligman"/> |
'''NGC 1783''' (also known as '''ESO 85-SC29''') is a [[globular cluster]] within the [[Dorado]] constellation and part of the [[Large Magellanic Cloud]], a satellite dwarf galaxy of the [[Milky Way]]. At an aperture of 50 arcseconds, its apparent V-band magnitude is 10.39,<ref name=Song/> making it one of the brightest globular clusters in the LMC as viewed from Earth. It was discovered in 1835 by [[John Herschel]]. The compiler of the [[New General Catalogue]], [[John Louis Emil Dreyer]], described this cluster as "considerably bright, large, round, very gradually pretty much brighter middle, mottled but not resolved."<ref name="cseligman"/> |
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NGC 1783 is about 1.7 billion years old. Its estimated mass is {{solar mass|{{val|9.8e4}}|link=y}}, and its total luminosity is {{solar luminosity|{{val|3.77e5}}|link=y}}, leading to a mass-to-luminosity ratio of 0.26 {{solar mass}}/{{solar luminosity}}.<ref name=Song>{{cite journal|doi=10.1093/mnras/stab1065|title=Dynamical masses and mass-to-light ratios of resolved massive star clusters – II. Results for 26 star clusters in the Magellanic Clouds|year=2021|last1=Song|first1=Ying-Yi|last2=Mateo|first2=Mario|last3=Bailey|first3=John I.|last4=Walker|first4=Matthew G.|last5=Roederer|first5=Ian U.|last6=Olszewski|first6=Edward W.|last7=Reiter|first7=Megan|last8=Kremin|first8=Anthony|journal=Monthly Notices of the Royal Astronomical Society|volume=504|issue=3|pages=4160–4191|arxiv=2104.06882}}</ref> All else equal, older star clusters have higher mass-to-luminosity ratios; that is, they have lower luminosities for the same mass.<ref name=Song/> |
NGC 1783 is about 1.7 billion years old. Its estimated mass is {{solar mass|{{val|9.8e4}}|link=y}}, and its total luminosity is {{solar luminosity|{{val|3.77e5}}|link=y}}, leading to a mass-to-luminosity ratio of 0.26 {{solar mass}}/{{solar luminosity}}.<ref name=Song>{{cite journal|doi=10.1093/mnras/stab1065|title=Dynamical masses and mass-to-light ratios of resolved massive star clusters – II. Results for 26 star clusters in the Magellanic Clouds|year=2021|last1=Song|first1=Ying-Yi|last2=Mateo|first2=Mario|last3=Bailey|first3=John I.|last4=Walker|first4=Matthew G.|last5=Roederer|first5=Ian U.|last6=Olszewski|first6=Edward W.|last7=Reiter|first7=Megan|last8=Kremin|first8=Anthony|journal=Monthly Notices of the Royal Astronomical Society|volume=504|issue=3|pages=4160–4191|doi-access=free |arxiv=2104.06882}}</ref> All else equal, older star clusters have higher mass-to-luminosity ratios; that is, they have lower luminosities for the same mass.<ref name=Song/> |
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==References== |
==References== |
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Latest revision as of 12:06, 18 July 2024
| NGC 1783 | |
|---|---|
 Hubble Space Telescope image of NGC 1783[1] | |
| Observation data (J2000 epoch) | |
| Constellation | Dorado[2] |
| Right ascension | 04h 59m 08.6s[3] |
| Declination | −65° 59′ 15.8″[3] |
| Distance | 160 Kly[4] (49 kpc[4]) |
| Apparent magnitude (V) | 10.93[5] |
| Apparent dimensions (V) | 5.3′ × 4.7′[3] |
| Physical characteristics | |
| Mass | 9.8×104[5] M☉ |
| Estimated age | 1.70±0.05 Gyr[5] |
| Other designations | ESO 85-SC29 |
NGC 1783 (also known as ESO 85-SC29) is a globular cluster within the Dorado constellation and part of the Large Magellanic Cloud, a satellite dwarf galaxy of the Milky Way. At an aperture of 50 arcseconds, its apparent V-band magnitude is 10.39,[5] making it one of the brightest globular clusters in the LMC as viewed from Earth. It was discovered in 1835 by John Herschel. The compiler of the New General Catalogue, John Louis Emil Dreyer, described this cluster as "considerably bright, large, round, very gradually pretty much brighter middle, mottled but not resolved."[2]
NGC 1783 is about 1.7 billion years old. Its estimated mass is 9.8×104 M☉, and its total luminosity is 3.77×105 L☉, leading to a mass-to-luminosity ratio of 0.26 M☉/L☉.[5] All else equal, older star clusters have higher mass-to-luminosity ratios; that is, they have lower luminosities for the same mass.[5]
References
[edit]- ^ "A youthful cluster". ESA/Hubble Picture of the Week. Retrieved 24 August 2015.
- ^ a b "New General Catalogue Objects: NGC 1750 - 1799". Retrieved 2015-09-20.
- ^ a b c "NGC 1783". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2015-09-20.
- ^ a b "NED results for object NGC 1783". NASA/IPAC Extragalactic Database. Retrieved 2015-09-20.
- ^ a b c d e f Song, Ying-Yi; Mateo, Mario; Bailey, John I.; Walker, Matthew G.; Roederer, Ian U.; Olszewski, Edward W.; Reiter, Megan; Kremin, Anthony (2021). "Dynamical masses and mass-to-light ratios of resolved massive star clusters – II. Results for 26 star clusters in the Magellanic Clouds". Monthly Notices of the Royal Astronomical Society. 504 (3): 4160–4191. arXiv:2104.06882. doi:10.1093/mnras/stab1065.
External links
[edit]
Media related to NGC 1783 at Wikimedia Commons
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