请输入您要查询的百科知识:

 

词条 NGC 1533
释义

  1. Notes

  2. References

  3. External links

{{Infobox Galaxy
| image = NGC 1533 .jpg
| image_size = 300px
| name = NGC 1533
| epoch = J2000
| type = (L)SB(rs)00[1]
| ra = {{RA|04|09|51.8}}[1]
| dec = {{DEC|-56|07|06}}[1]
| dist_ly = 62 ± 4 Mly (19.0 ± 1.1 Mpc)[4]{{Ref_label|A|a|none}}
| z = 790 ± 5 km/s[1]
| appmag_v = 11.7[1]
| size_v = 2′.8 × 2′.3[1]
| constellation name = Dorado
| notes =
| names = PGC 14582[1]
}}NGC 1533 is a barred lenticular galaxy with faint spiral structure in the constellation Dorado. The seventh-brightest member of the Dorado Group and 1°[9] off the group's center,[2] it is surrounded by a vast arc or ring of H I which is connected to IC 2038 and IC 2039.[2] The ring orbits around 32 kpc from the center.[3]{{Ref_label|B|b|none}} As is typical of lenticular galaxies, star formation is weak in NGC 1533.[2] Using both the surface brightness fluctuation (SBF) and globular cluster luminosity function (GCLF) methods, its distance was estimated in 2007 to be 19.4 ± 1.1 Mpc and 18.6 ± 2.0 Mpc respectively.[2] Averaging these together gives a distance of around 19 million parsecs or 62 million light-years from earth.{{Ref_label|A|a|none}} In 1970, a supernova was detected in NGC 1533.[4]

NGC 1533 was discovered by John Herschel on December 5, 1834.

Notes

{{refbegin}}
  1. {{Note_label|A|a|none}}average(19.4 ± 1.1, 18.6 ± 2.0) = ((19.4 + 18.6) / 2) ± ((1.12 + 2.02)0.5 / 2) = 19.0 ± 1.1
  2. {{Note_label|B|b|none}}35 kpc calculated assuming a distance of 21 Mpc[3] converts to a distance of 32 (35 ÷ 21 × 19) kpc for the current distance estimate of 19 Mpc
{{refend}}

References

1. ^{{cite web | title=NASA/IPAC Extragalactic Database | work=Results for NGC 1533 | url=http://nedwww.ipac.caltech.edu/ | accessdate=2008-06-26 }}
2. ^{{cite journal | author = DeGraaff, Regina Barber | author2 =Blakeslee, John P. | author3 =Meurer, Gerhardt R. | author4 =Putman, Mary E. | title = A Galaxy in Transition: Structure, Globular Clusters, and Distance of the Star-Forming S0 Galaxy NGC 1533 in Dorado | journal = The Astrophysical Journal | date = December 2007 | volume = 671 | issue = 2 | pages = 1624–1639 | url = http://www.iop.org/EJ/article/0004-637X/671/2/1624/72739.html | doi = 10.1086/523640| bibcode=2007ApJ...671.1624D| arxiv =0710.0893}}
3. ^{{Cite book | author = Ryan-Weber, Emma | author2 =Webster, Rachel | author3 =Bekki, Kenji | title = Galactic Recycling: The HI Ring Around NGC 1533 | journal = The IGM/Galaxy Connection: The Distribution of Baryons at Z=0, ASSL Conference Proceedings | editor = Jessica L. Rosenberg | editor2 = Mary E. Putman | publisher = Kluwer Academic Publishers | place = Dordrecht | date = April 2003 | volume = 281 | pages = 223 | bibcode = 2003ASSL..281..223R | isbn = 978-1-4020-1289-1 | postscript = |arxiv = astro-ph/0209321 |doi = 10.1007/978-94-010-0115-1_40 }}
4. ^{{cite journal | author = Evans, R. | title = Supernova in NGC 1533. | journal = IAU Circ. | date = 1970 | volume = 2279 | issue = 2279 | pages = 1 | bibcode = 1970IAUC.2279....1E }}

External links

  • {{WikiSky}}
  • Sky View image of NGC 1533
{{Sky|04|09|51.8|-|56|07|06|62000000}}{{Ngc20}}

8 : Barred lenticular galaxies|Dorado (constellation)|Dorado Group|Ring galaxies|NGC objects|Principal Galaxies Catalogue objects|Discoveries by John Herschel|Astronomical objects discovered in 1834

随便看

 

开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。

 

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间:2024/9/20 16:32:42