英文互译镜像站

3C 196.1

Last updated
3C 196.1
3C 196.1 PanSTARRS i.r.g.jpg
Radio galaxy 3C 196.1.
Observation data (J2000.0 epoch)
Constellation Hydra
Right ascension 08h 15m 27.810s
Declination −03° 08′ 26.61″
Redshift 0.198000
Heliocentric radial velocity 59,359 km/s
Distance 2.383 Gly
Apparent magnitude  (V)16.94
Apparent magnitude  (B)18.49
Characteristics
Type cD
Notable features Radio galaxy of HyMORS type, X-ray cavity
Other designations
LEDA 1075766, DA 247, NVSS J081527-030826, PKS 0812-029, 3CR 196.1, 4C -02.35, NRAO 286, TXS 0812-029

3C 196.1 is a low-excitation radio galaxy [1] [2] located in the constellation of Hydra. It has a redshift of 0.198 [3] and was first discovered as an astronomical radio source in 1965. [4] This object resides as the brightest cluster galaxy (BCG) of a cool core galaxy cluster CIZA J0815.4-0308 located at the same redshift, with its source being best described as a HyMOR (Hybrid Morphology Radio Source). [5] [6]

Contents

Description

The host galaxy of 3C 196.1 is a type-cD elliptical galaxy confirmed by near-infrared and optical imaging. It is described having an elongated structure from northeast and southwest direction [7] [8] with an estimated angular size of 3.16 kpc arcsec−1. [6] According to optical color gradients of the host galaxy, 3C 196.1 exhibits periodic shells with the centroids of the optical isotopes having a directional shift towards southwest, indicating a merger stage. [5] Furthermore, nucleus of the galaxy is partly obscured by interstellar dust [9] and appears to be split in several patches of emission that is extended along the nucleus' direction. [10]

Radio imaging of 3C 196.1 made by Very Large Array, shows a compact one-sided source within the host galaxy and a secondary nucleus on its side opposite its radio extension, [11] measuring a total size of 16 kpc and an orientation along a position angle of 40°. The southwest side of the galaxy has an enshrouded radio lobe with the region displaying high recessional velocities that is exceeding 500 km s−1 whereas the northwest side is more diffused with a small velocity dispersion. [12]

According to X-ray and radio imaging analysis, 3C 196.1 has a butterfly-shaped X-ray cavity located 10 kpc from its nucleus with the inner and outer cavities having jet power of 1.9 x 1044 erg s−1 and 3.4 x 1044 erg s−1 respectively. The enthalpies of the inner and outer cavities are computed as 7 x 1058 erg and 3 x 1060 erg. [5] Further evidence also shows presence of ionized gas filling up the cavity suggesting either the gas underwent numerous ionization events from AGN outbursts caused by the galaxy or the cooling of AGN outflows (104 < T ≤ 107 K) are causing the gas to form filaments. [8]

Related Research Articles

<span class="mw-page-title-main">3C 449</span> Radio galaxy in the constellation Lacerta

3C 449 is a low-redshift Fanaroff and Riley class I radio galaxy. It is thought to contain a highly warped circumnuclear disk surrounding the central active galactic nucleus (AGN). The name signifies that it was the 449th object of the Third Cambridge Catalog of Radio Sources (3C), published in 1959.

<span class="mw-page-title-main">3C 305</span> Galaxy in the constellation Draco

3C 305, also known as IC 1065, is a lenticular galaxy located in the constellation Draco. The galaxy is located 577 million light-years away from Earth. It has an active galactic nucleus and is classified as a Seyfert 2 galaxy. This galaxy was discovered by American astronomer Lewis Swift on April 7, 1888.

<span class="mw-page-title-main">3C 79</span> Galaxy in the constellation Aries

3C 79 is a Seyfert Galaxy and a radio galaxy located in the constellation Aries. It is hosted by an elliptical galaxy described as elongated with a complex morphology.

<span class="mw-page-title-main">3C 285</span> Galaxy in constellation Canes Venatici

3C 285 is a radio galaxy located in the constellation Canes Venatici. It is located about 1 bilion light years away. It is a Fanaroff-Riley 2 radio galaxy and is hosted in a disturbed spiral galaxy.

<span class="mw-page-title-main">3C 438</span> Galaxy in the constellation Cygnus

3C 438 is a Seyfert galaxy and Fanaroff and Riley class II radio galaxy located in the constellation Cygnus. The radio galaxy has two lobes and there is a radio jet leading to the south lobe, which also has a prominent double hot spot. There is age variation across the lobes.

<span class="mw-page-title-main">3C 236</span> Galaxy in the constellation Leo Minor

3C 236 is a Fanaroff and Riley Class II radio galaxy. It is among the largest known radio galaxies; the radio structure has a total linear size in excess of 4.5 Mpc. The galaxy features a "double-double" radio morphology consisting of the giant relic 4.5 Mpc source and an inner 2 kpc compact steep spectrum radio source. A recent starburst episode near the nucleus may be related to the event resulting in re-ignition of radio activity.

<span class="mw-page-title-main">Hercules A</span>

Hercules A is a bright astronomical radio source in the constellation Hercules corresponding to the galaxy 3C 348.

<span class="mw-page-title-main">NGC 3862</span> Galaxy in the constellation Leo

NGC 3862 is an elliptical galaxy located 300 million light-years away in the constellation Leo. Discovered by astronomer William Herschel on April 27, 1785, NGC 3862 is an outlying member of the Leo Cluster.

<span class="mw-page-title-main">NGC 708</span> Galaxy in the constellation Andromeda

NGC 708 is an elliptical galaxy located 240 million light-years away in the constellation Andromeda and was discovered by astronomer William Herschel on September 21, 1786. It is classified as a cD galaxy and is the brightest member of Abell 262. NGC 708 is a weak FR I radio galaxy and is also classified as a type 2 Seyfert galaxy.

<span class="mw-page-title-main">NGC 547</span> Galaxy in the constellation Cetus

NGC 547 is an elliptical galaxy and radio galaxy located in the constellation Cetus. It is located at a distance of about 220 million light years from Earth, which, given its apparent dimensions, means that NGC 547 is about 120,000 light years across. It was discovered by William Herschel on October 1, 1785. It is a member of the Abell 194 galaxy cluster and is included along with NGC 547 in the Atlas of Peculiar Galaxies.

<span class="mw-page-title-main">NGC 7237</span> Galaxy in the constellation Pegasus

NGC 7237 is an interacting lenticular galaxy located in the constellation Pegasus. It is located at a distance of about 350 million light years from Earth, which, given its apparent dimensions, means that NGC 7237 is about 240,000 light years across. NGC 7237 forms a pair with NGC 7236 and is a radio galaxy. It was discovered by Albert Marth on August 25, 1864.

<span class="mw-page-title-main">Extended emission-line region</span> Interstellar clouds

An extended emission-line region (EELR) is a giant interstellar cloud ionized by the radiation of an active galactic nucleus (AGN) inside a galaxy or photons produced by the shocks associated with the radio jets. An EELR can appear as a resolved cloud in relative nearby galaxies and as narrow emission lines in more distant galaxies.

<span class="mw-page-title-main">NGC 5920</span> Lenticular galaxy located in constellation Serpens

NGC 5920 is a large lenticular galaxy located in the Serpens constellation. Discovered on March 30, 1887, by American astronomer Lewis Swift, NGC 5920 is 711 million light-years distant from planet Earth. It is a narrow-line radio galaxy and about 300,000 light-years in diameter.

<span class="mw-page-title-main">4C+55.16</span> Seyfert 2 galaxy in the constellation Ursa Major

4C+55.16 is an elliptical galaxy, classified type E, located in Ursa Major. The galaxy lies about 2.84 billion light-years from Earth, which means given its apparent dimensions, 4C+55.16 is approximately 445,000 light-years across making it a type-cD galaxy. It is the brightest cluster galaxy (BCG) in a cluster of the same name.

<span class="mw-page-title-main">3C 346</span> Galaxy in the constellation Hercules

3C 346 is an elliptical galaxy located in the constellation Hercules. It is located nearly 2.5 billion light years away from Earth and classified a Seyfert galaxy and a compact steep-spectrum source (CSS), although later studies confirm it as a Fanaroff-Riley class II source.

<span class="mw-page-title-main">3C 459</span> Radio galaxy in the constellation Pisces

3C 459 known as IRAS 23140+0348, is a radio galaxy located in the constellation Pisces. It is located 2.74 billion light years from Earth and is classified as a Seyfert 2 and LINER galaxy.

<span class="mw-page-title-main">3C 138</span> Quasar in the constellation Taurus

3C 138 is a quasar located in the constellation of Taurus. It has a redshift of (z) 0.76. The radio spectrum of this source appears both compact and steep, making it a compact steep-spectrum radio quasar. It is also one of the few 3C objects showing a defined and turn-over in its electromagnetic spectrum at low frequencies.

<span class="mw-page-title-main">3C 309.1</span> Quasar in the constellation Ursa Minor

3C 309.1 is a quasar located in the constellation of Ursa Minor. It has a redshift (z) of 0.90 and was first identified as an astronomical radio source from the Third Cambridge Catalogue of Radio Sources by in 1966. This object contains a compact steep spectrum (CSS) source, and is classified as one of the brightest and largest of its kind.

<span class="mw-page-title-main">3C 356</span> Radio galaxy in the constellation Draco

3C 356 is a distant radio galaxy located in the constellation of Draco, hosted by a merging pair of elliptical galaxies located at redshift (z) 1.079 with two radio cores having a separation gap of 5 arcseconds. It was first discovered as an astronomical radio source by P. Veron from a 3C revised catalogue in 1966 and such, shows an alignment effect at both wavelengths. The X-ray source luminosity for this galaxy is estimated to be 2.5 x 1044 erg s−1.

<span class="mw-page-title-main">3C 382</span> Broad-line radio galaxy located in the constellation Lyra

3C 382 is a nearby broad-line radio galaxy located in the constellation of Lyra, located at a redshift of (z) 0.058. First discovered as an astronomical radio source in 1963 and identified with its optical counterpart in 1973, the galaxy is classified as a Fanaroff-Riley class II radio galaxy. Its X-ray luminosity is estimated to be 7×1044 erg/s in the 0.2–2.4 keV band.

References

  1. ↑ Ricci, Federica (2022-09-01). "Dissecting the stormy weather in 3C 196.1". Chandra Proposal: 6381. Bibcode:2022cxo..prop.6381R.
  2. ↑ Jimenez-Gallardo, Ana; Massaro, Francesco; Sani, Eleonora; Mazzucchelli, Chiara; Ricci, Federica; Balmaverde, Barbara; Capetti, Alessandro; Forman, William; Kraft, Ralph; Venturi, Giacomo; Prieto, Almudena; Marconi, Alessandro; Baum, Stefi; O'Dea, Chris; Paggi, Alessandro (2022-07-01). "Feedback on radio galaxies: the cases of 3CR 318.1 and 3CR 196.1". 44th COSPAR Scientific Assembly. Held 16–24 July. 44: 2328. Bibcode:2022cosp...44.2328J.
  3. ↑ Balmaverde, B.; Capetti, A.; Baldi, R. D.; Baum, S.; Chiaberge, M.; Gilli, R.; Jimenez-Gallardo, A.; Marconi, A.; Massaro, F.; Meyer, E.; O’Dea, C.; Speranza, G.; Torresi, E.; Venturi, G. (June 2022). "The MURALES survey VI. Properties and origin of the extended line emission structures in radio galaxies". Astronomy & Astrophysics. 662: A23. arXiv: 2204.00528 . Bibcode:2022A&A...662A..23B. doi:10.1051/0004-6361/202142823. ISSN   0004-6361.
  4. ↑ Conway, R. G.; Daintree, E. J.; Long, R. J. (1965-12-01). "Observations of Radio Sources at 612 and 1 400 Mc/s". Monthly Notices of the Royal Astronomical Society. 131 (1): 159–171. doi: 10.1093/mnras/131.1.159 . ISSN   0035-8711.
  5. 1 2 3 Ricci, F.; Lovisari, L.; Kraft, R. P.; Massaro, F.; Paggi, A.; Liuzzo, E.; Tremblay, G.; Forman, W. R.; Baum, S.; O’Dea, C.; Wilkes, B. (October 2018). "Stormy Weather in 3C 196.1: Nuclear Outbursts and Merger Events Shape the Environment of the Hybrid Radio Galaxy 3C 196.1". The Astrophysical Journal. 867 (1): 35. arXiv: 1809.10693 . Bibcode:2018ApJ...867...35R. doi: 10.3847/1538-4357/aae487 . ISSN   0004-637X.
  6. 1 2 Massaro, F.; Tremblay, G. R.; Harris, D. E.; Kharb, P.; Axon, D.; Balmaverde, B.; Baum, S. A.; Capetti, A.; Chiaberge, M.; Gilli, R.; Giovannini, G.; Grandi, P.; Macchetto, F. D.; O'Dea, C. P.; Risaliti, G. (2012-11-28). "CHANDRA OBSERVATIONS OF 3C RADIO SOURCES WITH z< 0.3. II. COMPLETING THE SNAPSHOT SURVEY". The Astrophysical Journal Supplement Series. 203 (2): 31. arXiv: 1210.6027 . Bibcode:2012ApJS..203...31M. doi:10.1088/0067-0049/203/2/31. ISSN   0067-0049.
  7. ↑ Madrid, Juan P.; Chiaberge, Marco; Floyd, David; Sparks, William B.; Macchetto, Duccio; Miley, George K.; Axon, David; Capetti, Alessandro; O’Dea, Christopher P.; Baum, Stefi; Perlman, Eric; Quillen, Alice (June 2006). "Hubble Space Telescope Near-Infrared Snapshot Survey of 3CR Radio Source Counterparts at Low Redshift". The Astrophysical Journal Supplement Series. 164 (2): 307–333. arXiv: astro-ph/0603239 . Bibcode:2006ApJS..164..307M. doi:10.1086/504480. ISSN   0067-0049.
  8. 1 2 Jimenez-Gallardo, A.; Sani, E.; Ricci, F.; Mazzucchelli, C.; Balmaverde, B.; Massaro, F.; Capetti, A.; Forman, W. R.; Kraft, R. P.; Venturi, G.; Gendron-Marsolais, M.; Prieto, M. A.; Marconi, A.; Peña-Herazo, H. A.; Baum, S. A. (2022-12-01). "The Cavity of 3CR 196.1: Hα Emission Spatially Associated with an X-Ray Cavity". The Astrophysical Journal. 941 (2): 114. arXiv: 2211.04481 . Bibcode:2022ApJ...941..114J. doi: 10.3847/1538-4357/aca08b . ISSN   0004-637X.
  9. ↑ de Koff, Sigrid; Best, Philip; Baum, Stefi A.; Sparks, William; Rottgering, Huub; Miley, George; Golombek, Daniel; Macchetto, Ferdinando; Martel, Andre (July 2000). "The Dust-Radio Connection in 3CR Radio Galaxies". The Astrophysical Journal Supplement Series. 129 (1): 33–159. Bibcode:2000ApJS..129...33D. doi:10.1086/313402.
  10. ↑ de Koff, Sigrid; Baum, Stefi A.; Sparks, William B.; Biretta, John; Golombek, Daniel; Macchetto, Ferdinando; McCarthy, Patrick; Miley, George K. (December 1996). "HST Snapshot Survey of 3CR Radio Source Counterparts. I. Intermediate Redshifts". The Astrophysical Journal Supplement Series. 107 (2): 621–660. Bibcode:1996ApJS..107..621D. doi:10.1086/192376. ISSN   0067-0049.
  11. ↑ Neff, S. G.; Roberts, L.; Hutchings, J. B. (1995-08-01). "VLA Maps of Radio Galaxies to Z = 1". The Astrophysical Journal Supplement Series. 99: 349. Bibcode:1995ApJS...99..349N. doi:10.1086/192190. ISSN   0067-0049.
  12. ↑ Balmaverde, B.; Capetti, A.; Marconi, A.; Venturi, G.; Chiaberge, M.; Baldi, R. D.; Baum, S.; Gilli, R.; Grandi, P.; Meyer, E. T.; Miley, G.; O’Dea, C.; Sparks, W.; Torresi, E.; Tremblay, G. (2020-12-21). "The MURALES survey III. Completing the MUSE observations of 37 3C low-z radio galaxies". Astronomy & Astrophysics. 645: A12. arXiv: 2010.11195 . doi:10.1051/0004-6361/202039062. ISSN   0004-6361.
This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.
镜像程序 整站镜像下载 蚂蚁镜像站群 递归网站下载 整站下载器