Misplaced Pages

NGC 4526: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editContent deleted Content addedVisualWikitext
Revision as of 18:54, 24 October 2021 editJMK (talk | contribs)Autopatrolled, Extended confirmed users27,503 edits notoc← Previous edit Latest revision as of 04:50, 3 December 2024 edit undoPhantomdj (talk | contribs)Extended confirmed users2,426 editsm updated SN info 
(20 intermediate revisions by 14 users not shown)
Line 3: Line 3:
| name = ] 4526 | name = ] 4526
| image = ] | image = ]
| caption = Supernova ] (lower left) in the outskirts of NGC 4526 | caption = Supernova ] (lower left) in the outskirts of NGC 4526's central disk
| epoch = ] | epoch = ]
| type = SAB(s)0°<ref name="Burstein1979"/> | type = SAB(s)0°<ref name="Burstein1979"/>
| ra = {{RA|12|34|03.029}}<ref name="ApJ131_1163"/> | ra = {{RA|12|34|03.029}}<ref name="ApJ131_1163"/>
| dec = {{DEC|+07|41|56.90}}<ref name="ApJ131_1163"/> | dec = {{DEC|+07|41|56.90}}<ref name="ApJ131_1163"/>
| dist_ly = {{val|55|5|ul=Mly}}&nbsp;({{val|16.9|1.6|ul=Mpc}})<ref name="tonryetal2001"/> | dist_ly = {{val|55|5|ul=Mly}}&nbsp;({{val|16.9|1.6|ul=Mpc}})<ref name="tonryetal2001"/><br/>{{convert|15.8|Mpc|Mly|abbr=on|lk=on|order=flip}}<ref name=Hatt_et_al_2018/>
| z = {{val|0.001494|0.000027}} | z = {{val|0.001494|0.000027}}
| h_radial_v = {{val|448|8|u=km/s}}<ref name="ned" /> | h_radial_v = {{val|448|8|u=km/s}}<ref name="ned" />
Line 14: Line 14:
| size_v = {{nowrap|7′.2 × 2′.4}}<ref name="ned" /> | size_v = {{nowrap|7′.2 × 2′.4}}<ref name="ned" />
| constellation name = ] | constellation name = ]
| names = ] 4560,<ref name="ned" /> ] 7718,<ref name="ned" /> ] 41772<ref name="ned" /> | names = {{odlist | NGC= 4560 | UGC= 7718 | PGC= 41772 | CGCG= 042-155 | MCG= +01-32-100 | IRAS= 12315+0758}}<ref name="ned" />
}} __NOTOC__ }} __NOTOC__


'''NGC 4526''' (also listed as '''NGC 4560''') is a ] located approximately 55 million ]s from the ]<ref name="tonryetal2001"/> in the ] ] and discovered on 13 April 1784 by ].<ref name=cseligman>{{cite web|title=New General Catalog Objects: NGC 4500 - 4549|url=https://cseligman.com/text/atlas/ngc45.htm#4526|author=Courtney Seligman|access-date=October 17, 2021}}</ref> '''NGC 4526''' (also listed as '''NGC 4560''') is a ] with an embedded dusty disc, located approximately 55 million ]s from the ]<ref name="tonryetal2001"/> in the ] ] and discovered on 13 April 1784 by ].<ref name=cseligman>{{cite web|title=New General Catalog Objects: NGC 4500 - 4549|url=https://cseligman.com/text/atlas/ngc45.htm#4526|author=Courtney Seligman|access-date=October 17, 2021}}</ref> Herschel observed it again on 28 December 1785, resulting in the galaxy being entered twice into the ].<ref name=cseligman />


The galaxy is seen nearly edge-on. The ] is SAB(s)0°,<ref name="Burstein1979"/> which indicates a lenticular structure with a weak bar across the center and pure ]s without a ring.<ref name="Buta2007"/> It belongs to the ] and is one of the brightest known lenticular galaxies.<ref name="Burstein1979"/> The galaxy is seen nearly edge-on. The ] is SAB(s)0°,<ref name="Burstein1979"/> which indicates a lenticular structure with a weak bar across the center and pure ]s without a ring.<ref name="Buta2007"/> It belongs to the ] and is one of the brightest known lenticular galaxies.<ref name="Burstein1979"/>
In the galaxy's outer halo, ] orbital velocities<ref>{{cite journal | author1=Adebusola B. Alabi | author2=Duncan A. Forbes | author3=Aaron J. Romanowsky |author4=Jean P. Brodie | author5=Jay Strader | author6=Joachim Janz | author7=Christopher Usher | author8=Lee R. Spitler | author9=Sabine Bellstedt | author10=Anna Ferre-Mateu | title=The SLUGGS survey: the mass distribution in early-type galaxies within five effective radii and beyond | journal=Monthly Notices of the Royal Astronomical Society | volume=460 | issue=4 | date=2016-05-20 | pages=3838–3860 | doi=10.1093/mnras/stw1213 | doi-access=free | bibcode=2016MNRAS.460.3838A | arxiv=1605.06101 | s2cid=55054073 }}</ref> indicate abnormal poverty of dark matter: only 43±18% of the mass within 5 ].
In the galaxy's outer halo,
] orbital velocities<ref>{{cite journal
|author1=Adebusola B. Alabi
|author2=Duncan A. Forbes
|author3=Aaron J. Romanowsky
|author4=Jean P. Brodie
|author5=Jay Strader
|author6=Joachim Janz
|author7=Christopher Usher
|author8=Lee R. Spitler
|author9=Sabine Bellstedt
|author10=Anna Ferre-Mateu
|title=The SLUGGS survey: the mass distribution in early-type galaxies within five effective radii and beyond
|journal=Monthly Notices of the Royal Astronomical Society
|volume=460
|issue=4
|date=2016-05-20
|pages=3838–3860
|doi=10.1093/mnras/stw1213
|bibcode=2016MNRAS.460.3838A
|arxiv=1605.06101 |s2cid=55054073
}}</ref>
indicate abnormal poverty of dark matter:
only 43±18% of the mass within 5 ].


The inner nucleus of this galaxy displays a rise in stellar orbital motion that indicates the presence of a central dark mass. The best fit model for the motion of molecular gas in the core region suggests there is a ] with about {{val|4.5|+4.2|-3.0|e=8}} (450 million) times the ].<ref name="nature494_7437_328"/> This is the first object to have its black-hole mass estimated by measuring the rotation of gas molecules around its centre with an ] (in this case the ]). The inner nucleus of this galaxy displays a rise in stellar orbital motion that indicates the presence of a central dark mass. The best fit model for the motion of molecular gas in the core region suggests there is a ] with about {{val|4.5|+4.2|-3.0|e=8}} (450 million) times the ].<ref name="nature494_7437_328"/> This is the first object to have its black-hole mass estimated by measuring the rotation of gas molecules around its centre with an ] (in this case the ]).


==Supernovae==
Supernova ] was discovered in this galaxy in 1969, reaching a peak magnitude of 16.<ref name="KowalSargent1971"/> In 1994, a ] was discovered about two weeks before reaching peak brightness. Designated ], it was caused by the explosion of a ] star composed of carbon and oxygen.<ref name="Lentz2001"/>
Two ]e have been observed in NGC 4526:
* SN 1969E (type unknown, mag. 16) was discovered by Enrique Chavira on 23 March 1969.<ref>{{cite web
| url = http://www.cbat.eps.harvard.edu/IAUCs/IAUC2139.jpg
| title = Circular No. 2139
| last = Gingerich
| first = Owen
| date = 27 March 1969
| website = Central Bureau for Astronomical Telegrams
| publisher = Smithsonian Astrophysical Observatory
| access-date = 2 December 2024
}}</ref><ref name="KowalSargent1971"/>
* ] (], mag. 15.2) was discovered independently by the ] Supernova Search and by Dr. M. Richmond, on 7 March 1994, about two weeks before reaching peak brightness.<ref>{{cite journal | bibcode = 1994IAUC.5946....2T| title = Supernova 1994D in NGC 4526| last1 = Treffers| first1 = R. R.| last2 = Filippenko| first2 = A. V.| last3 = Van Dyk| first3 = S. D.| last4 = Richmond| first4 = M. W.| last5 = Martel| first5 = A.| last6 = Goodrich| first6 = R. W.| journal = International Astronomical Union Circular| date = 1994| issue = 5946| page = 2}}</ref> It was caused by the explosion of a ] star composed of carbon and oxygen.<ref name="Lentz2001"/>


] image showing the envelope of more distant orbiting stars]]
==Gallery==
<gallery>
File:NGC4526 - SDSS DR14 (panorama).jpg|NGC 4526 as photographed by the ].<ref>{{cite web|title=The whirling disc of NGC 4526|url=http://www.spacetelescope.org/images/potw1442a/|website=www.spacetelescope.org|publisher=ESA/Hubble|access-date=20 October 2014}}</ref>
</gallery>


==See also== ==See also==
Line 98: Line 84:
| doi = 10.1086/111193 | doi = 10.1086/111193
| postscript= . | postscript= .
| doi-access= free
}}</ref>
}}</ref>


<ref name="Lentz2001">{{citation <ref name="Lentz2001">{{citation
Line 133: Line 120:
| doi = 10.1086/190625 | doi = 10.1086/190625
| postscript= . | postscript= .
| doi-access= free
}}</ref>
}}</ref>


<ref name="tonryetal2001">{{citation <ref name="tonryetal2001">{{citation
Line 158: Line 146:
}}</ref> }}</ref>


<ref name="ApJ131_1163">{{cite journal |doi=10.1086/498708 |last1=Skrutskie |first1=Michael F. |last2=Cutri |first2=Roc M. |last3=Stiening |first3=Rae |last4=Weinberg |first4=Martin D. |last5=Schneider |first5=Stephen E. |last6=Carpenter |first6=John M. |last7=Beichman |first7=Charles A. |last8=Capps |first8=Richard W. |last9=Chester |first9=Thomas |last10=Elias |first10=Jonathan H. |last11=Huchra |first11=John P. |last12=Liebert |first12=James W. |last13=Lonsdale |first13=Carol J. |last14=Monet |first14=David G. |last15=Price |first15=Stephan |last16=Seitzer |first16=Patrick |last17=Jarrett |first17=Thomas H. |last18=Kirkpatrick |first18=J. Davy |last19=Gizis |first19=John E. |last20=Howard |first20=Elizabeth V. |last21=Evans |first21=Tracey E. |last22=Fowler |first22=John W. |last23=Fullmer |first23=Linda |last24=Hurt |first24=Robert L. |last25=Light |first25=Robert M. |last26=Kopan |first26=Eugene L. |last27=Marsh |first27=Kenneth A. |last28=McCallon |first28=Howard L. |last29=Tam |first29=Robert |last30=Van Dyk |first30=Schuyler D. |last31=Wheelock |first31=Sherry L. |title=The Two Micron All Sky Survey (2MASS) |journal=The Astronomical Journal |date=1 February 2006 |volume=131 |issue=2 |pages=1163–1183 |bibcode=2006AJ....131.1163S |s2cid=18913331 |issn=0004-6256 |doi-access=free }}</ref>
<ref name="ApJ131_1163">{{Citation
| first1 = M. F. | last1 = Skrutskie
| first2 = R. M. | last2 = Cutri
| first3 = R. | last3 = Stiening
| first4 = M. D. | last4 = Weinberg
| first5 = S. | last5 = Schneider
| first6 = J. M. | last6 = Carpenter
| first7 = C. | last7 = Beichman
| first8 = R. | last8 = Capps
| first9 = T. | last9 = Chester
| first10 = J. | last10 = Elias
| first11 = J. | last11 = Huchra
| first12 = J. | last12 = Liebert
| first13 = C. | last13 = Lonsdale
| first14 = D. G. | last14 = Monet
| first15 = S. | last15 = Price
| first16 = P. | last16 = Seitzer
| first17 = T. | last17 = Jarrett
| first18 = J. D. | last18 = Kirkpatrick
| first19 = J. E. | last19 = Gizis
| first20 = E. | last20 = Howard
| first21 = T. | last21 = Evans
| first22 = J. | last22 = Fowler
| first23 = L. | last23 = Fullmer
| first24 = R. | last24 = Hurt
| first25 = R. | last25 = Light
| first26 = E. L. | last26 = Kopan
| first27 = K. A. | last27 = Marsh
| first28 = H. L. | last28 = McCallon
| first29 = R. | last29 = Tam
| first30 = S. | last30 = Van Dyk
| first31 = S. | last31 = Wheelock
| display-authors = 1
| title = The Two Micron All Sky Survey (2MASS)
| journal = Astronomical Journal
| volume = 131
| issue = 2
| pages = 1163–1183
|date=February 2006
| doi = 10.1086/498708
| bibcode = 2006AJ....131.1163S
| postscript = .
| doi-access = free
}}</ref>


<ref name="nature494_7437_328">{{citation <ref name="nature494_7437_328">{{citation
| last1 = Davis | last1 = Davis
| first1 = Timothy A. | first1 = Timothy A.
| last2 = Bureau | last2 = ((Bureau))
| first2 = Martin | first2 = Martin
| last3 = Cappellari | last3 = Cappellari
Line 228: Line 173:
| s2cid = 205232307 | s2cid = 205232307
}}</ref> }}</ref>

<ref name=Hatt_et_al_2018>{{cite journal
| title=The Carnegie-Chicago Hubble Program. IV. The Distance to NGC 4424, NGC 4526, and NGC 4356 via the Tip of the Red Giant Branch
| display-authors=1 | last1=Hatt | first1=Dylan
| last2=Freedman | first2=Wendy L. | last3=Madore | first3=Barry F.
| last4=Beaton | first4=Rachael L. | last5=Hoyt | first5=Taylor J.
| last6=Jang | first6=In Sung | last7=Lee | first7=Myung Gyoon
| last8=Monson | first8=Andrew J. | last9=Rich | first9=Jeffrey A.
| last10=Scowcroft | first10=Victoria | last11=Seibert | first11=Mark
| journal=The Astrophysical Journal
| volume=861 | issue=2 | id=104 | pages=10 | date=July 2018
| doi=10.3847/1538-4357/aac9cc | arxiv=1806.02900
| bibcode=2018ApJ...861..104H | s2cid=119430198 | doi-access=free }}</ref>

}} }}


Line 235: Line 194:
* *
* *



{{Ngc50}} {{Ngc50}}
Line 249: Line 207:
] ]
] ]
] ]
] ]
]
]
]

Latest revision as of 04:50, 3 December 2024

Lenticular galaxy in the constellation Virgo
NGC 4526
NGC 4526 with SN 1994D @ bottom leftSupernova SN 1994D (lower left) in the outskirts of NGC 4526's central disk
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension12 34 03.029
Declination+07° 41′ 56.90″
Redshift0.001494±0.000027
Heliocentric radial velocity448±8 km/s
Distance55±5 Mly (16.9±1.6 Mpc)
52 Mly (15.8 Mpc)
Apparent magnitude (V)10.7
Characteristics
TypeSAB(s)0°
Apparent size (V)7′.2 × 2′.4
Other designations
IRAS 12315+0758, NGC 4560, UGC 7718, MCG +01-32-100, PGC 41772, CGCG 042-155

NGC 4526 (also listed as NGC 4560) is a lenticular galaxy with an embedded dusty disc, located approximately 55 million light-years from the Solar System in the Virgo constellation and discovered on 13 April 1784 by William Herschel. Herschel observed it again on 28 December 1785, resulting in the galaxy being entered twice into the New General Catalogue.

The galaxy is seen nearly edge-on. The morphological classification is SAB(s)0°, which indicates a lenticular structure with a weak bar across the center and pure spiral arms without a ring. It belongs to the Virgo cluster and is one of the brightest known lenticular galaxies. In the galaxy's outer halo, globular cluster orbital velocities indicate abnormal poverty of dark matter: only 43±18% of the mass within 5 effective radii.

The inner nucleus of this galaxy displays a rise in stellar orbital motion that indicates the presence of a central dark mass. The best fit model for the motion of molecular gas in the core region suggests there is a supermassive black hole with about 4.5+4.2
−3.0×10 (450 million) times the mass of the Sun. This is the first object to have its black-hole mass estimated by measuring the rotation of gas molecules around its centre with an astronomical interferometer (in this case the Combined Array for Research in Millimeter-wave Astronomy).

Supernovae

Two supernovae have been observed in NGC 4526:

  • SN 1969E (type unknown, mag. 16) was discovered by Enrique Chavira on 23 March 1969.
  • SN 1994D (type Ia, mag. 15.2) was discovered independently by the Leuschner Observatory Supernova Search and by Dr. M. Richmond, on 7 March 1994, about two weeks before reaching peak brightness. It was caused by the explosion of a white dwarf star composed of carbon and oxygen.
Wider Hubble Space Telescope image showing the envelope of more distant orbiting stars

See also

References

  1. ^ Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  2. ^ "NASA/IPAC Extragalactic Database", Results for NGC 4526, retrieved 2006-10-18.
  3. ^ Tonry, J. L.; et al. (2001), "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances", Astrophysical Journal, 546 (2): 681–693, arXiv:astro-ph/0011223, Bibcode:2001ApJ...546..681T, doi:10.1086/318301, S2CID 17628238.
  4. Hatt, Dylan; et al. (July 2018). "The Carnegie-Chicago Hubble Program. IV. The Distance to NGC 4424, NGC 4526, and NGC 4356 via the Tip of the Red Giant Branch". The Astrophysical Journal. 861 (2): 10. arXiv:1806.02900. Bibcode:2018ApJ...861..104H. doi:10.3847/1538-4357/aac9cc. S2CID 119430198. 104.
  5. ^ Burstein, D. (November 1979), "Structure and origin of S0 galaxies. I - Surface photometry of S0 galaxies", Astrophysical Journal Supplement Series, 41: 435–450, Bibcode:1979ApJS...41..435B, doi:10.1086/190625.
  6. ^ Courtney Seligman. "New General Catalog Objects: NGC 4500 - 4549". Retrieved October 17, 2021.
  7. Buta, Ronald J.; et al. (2007), Atlas of Galaxies, Cambridge University Press, pp. 13–17, ISBN 978-0521820486.
  8. Adebusola B. Alabi; Duncan A. Forbes; Aaron J. Romanowsky; Jean P. Brodie; Jay Strader; Joachim Janz; Christopher Usher; Lee R. Spitler; Sabine Bellstedt; Anna Ferre-Mateu (2016-05-20). "The SLUGGS survey: the mass distribution in early-type galaxies within five effective radii and beyond". Monthly Notices of the Royal Astronomical Society. 460 (4): 3838–3860. arXiv:1605.06101. Bibcode:2016MNRAS.460.3838A. doi:10.1093/mnras/stw1213. S2CID 55054073.
  9. Davis, Timothy A.; et al. (February 2013), "A black-hole mass measurement from molecular gas kinematics in NGC4526", Nature, 494 (7437): 328–330, arXiv:1301.7184, Bibcode:2013Natur.494..328D, doi:10.1038/nature11819, PMID 23364690, S2CID 205232307.
  10. Gingerich, Owen (27 March 1969). "Circular No. 2139". Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory. Retrieved 2 December 2024.
  11. Kowal, C. T.; Sargent, W. L. W. (November 1971), "Supernovae discovered since 1885", Astronomical Journal, 41: 756–764, Bibcode:1971AJ.....76..756K, doi:10.1086/111193.
  12. Treffers, R. R.; Filippenko, A. V.; Van Dyk, S. D.; Richmond, M. W.; Martel, A.; Goodrich, R. W. (1994). "Supernova 1994D in NGC 4526". International Astronomical Union Circular (5946): 2. Bibcode:1994IAUC.5946....2T.
  13. Lentz, Eric J.; et al. (August 2001), "Non-LTE Synthetic Spectral Fits to the Type Ia Supernova 1994D in NGC 4526", The Astrophysical Journal, 557 (1): 756–764, arXiv:astro-ph/0104225, Bibcode:2001ApJ...557..266L, doi:10.1086/322239, S2CID 119535927.

External links

New General Catalogue 4500 to 4999
Astronomical catalogs
NGC
PGC
Constellation of Virgo
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Galaxies
Messier
NGC
Other
Galaxy clusters
Astronomical events
Category
Portals: Categories: