B2 0902+34
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| B2 0902+34 | |
|---|---|
| Observation data (J2000.0 epoch) | |
| Constellation | Lynx |
| Right ascension | 09h 05m 30.10s |
| Declination | +34° 07′ 56.92″ |
| Redshift | 3.395 |
| Heliocentric radial velocity | 1,013,898 km/s |
| Distance | 11.440 Gly (light travel time-distance) |
| Apparent magnitude (V) | 23.80 |
| Apparent magnitude (B) | 24.0 |
| Characteristics | |
| Type | Radio galaxy HEG |
| Other designations | |
| NVSS J090530.1+340756, 7C 0902+3420, TXS 0902+343, VLSS J0905.5+3407, 87GB 090225.3+341952, IVS B0902+343 | |
B2 0902+34 is a radio galaxy located in the constellation of Lynx. The redshift of the object is (z) 3.395[1] and it was discovered in October 1988, by S. J. Lilly who identified its astronomical radio source with a faint galaxy counterpart, making it the most distant when found at that period.[2]
B2 0902+34 is classified as a high redshift radio galaxy with a small radio source.[3][4] Its radio structure is bizarre with a long radio emission plume described as extending beyond the hot spot regions located in northern direction. There is a bright jet found having a knotty appearance with an extent of 1.5 arcseconds in length. Radio imaging showed the jet has a bending angle of almost 90° at its northern end, while the source's southern half shows two distinctive components separated by 1 arcsecond from each other.[4] A flat-spectrum radio core is located between the optical peaks, in a valley area.[5] The most interesting feature of B2 0902+34, are the large observed rotation measures and rotation gradients, as seen in the northern hot spot region, by multifrequency polarized imaging.[4] A fuzzy emission region is located north-east of the galaxy's two regions according to Hubble Space Telescope imaging.[6]
Observations by Very Large Array made in February 2024, showed there are detections of absorption lines due to presence of carbon monoxide and cyano radical elements, associated together with B2 0902+34. The carbon absorption of the galaxy has two components with one of them located at the same redshift as the 21 centimeter neutral hydrogen gas absorption.[7] Non-continuum emission at 2.9 millimeters was detected as well apart from carbon absorption, with source coinciding with a component seen on centimeter wavelengths. This component is likely interpreted as either the nucleus or the base of the jet.[8]
It is theorized B2 0902+34 might be a giant elliptical protogalaxy based on its spectrum, its luminosity of its continuum source, and the fact it shows a collapsing structure and large quantity of interstellar gas.[9][10] Apart from that, the galaxy has a Lyman-alpha emission halo with an extended radius of 50 kiloparsecs and velocity dispersion of 250 kilometer per seconds. Located in its spatially resolved region, a second feature is detected with a blueshifted line profile. It is suggested as either H I absorption or secondary emission.[10] According to studies, the galaxy is undergoing a wave of star formation which started 3 billion years ago.[11]
An observation by Chandra X-ray Observatory found B2 0902+34 is an obscured active galaxy. Based on studies, it has an unresolved X-ray source located in the center of its active galactic nucleus, with the spectrum of the source having well-fitted power law photon index measuring Γ~ 1.1 and intrinsic luminosity of 3.3 × 1045 erg s−1.[12] A large emission-line nebula is seen surrounding the galaxy, extending 10" × 8" on the sky's projection.[13]
References
- ↑ Eisenhardt, Peter; Dickinson, Mark (November 1992). "How Old Is the Z = 3.4 Radio Galaxy B2 0902+34". The Astrophysical Journal. 399: L47. Bibcode:1992ApJ...399L..47E. doi:10.1086/186603. ISSN 0004-637X.
- ↑ Lilly, S. J. (October 1988). "Discovery of a Radio Galaxy at a Redshift of 3.395". The Astrophysical Journal. 333: 161. Bibcode:1988ApJ...333..161L. doi:10.1086/166732. ISSN 0004-637X.
- ↑ Carilli, C. L.; Owen, F. N.; Harris, D. E. (February 1994). "Radio Continuum Polarimetric Imaging of High Redshift Radio Galaxies". The Astronomical Journal. 107: 480. Bibcode:1994AJ....107..480C. doi:10.1086/116870. ISSN 0004-6256.
- 1 2 3 Carilli, C. L. (June 1995). "The bizarre structure of the z=3.4 radio galaxy B2 0902 + 343". Astronomy and Astrophysics. 298: 77. Bibcode:1995A&A...298...77C. ISSN 0004-6361.
- ↑ Cordun, C. M.; Timmerman, R.; Miley, G. K.; Weeren, R. J. van; Sweijen, F.; Morabito, L. K.; Röttgering, H. J. A. (2023-08-01). "VLBI imaging of high-redshift galaxies and protoclusters at low radio frequencies with the International LOFAR Telescope". Astronomy & Astrophysics. 676: A29. arXiv:2306.00071. Bibcode:2023A&A...676A..29C. doi:10.1051/0004-6361/202346320. hdl:1887/3717310. ISSN 0004-6361.
- ↑ Pentericci, L.; Rottgering, H. J. A.; Miley, G. K.; McCarthy, P.; Spinrad, H.; Breugel, W. J. M. van; Macchetto, F. (1998-09-05), HST images and properties of the most distant radio galaxies, arXiv:astro-ph/9809056
- ↑ Emonts, Bjorn H. C.; Curran, Steve J.; Miley, George K.; Lehnert, Matthew D.; Carilli, Chris L.; Yoon, Ilsang; Morganti, Raffaella; van Weeren, Reinout J.; Villar-Martín, Montserrat; Guillard, Pierre; Cordun, Cristina M.; Oosteroo, Tom A. (2024-02-01). "Absorption of Millimeter-band CO and CN in the Early Universe: Molecular Clouds in the Radio Galaxy B2 0902+34 at Redshift 3.4". The Astrophysical Journal. 962 (2): 187. arXiv:2401.03577. Bibcode:2024ApJ...962..187E. doi:10.3847/1538-4357/ad198d. ISSN 0004-637X.
- ↑ Downes, D.; Solomon, P. M.; Sanders, D. B.; Evans, A. S. (September 1996). "Non-thermal mm-continuum emission from the radio galaxy B2 0902+343, and non-detection of CO(4-3)". Astronomy and Astrophysics. 313: 91–95. Bibcode:1996A&A...313...91D. ISSN 0004-6361.
- ↑ Eales, Steve; Rawlings, Steve; Puxley, Phil; Rocca-Volmerange, Brigitte; Kuntz, Kip (May 1993). "Evidence that the z = 3.4 radio galaxy B2 0902+34 may be a protogalaxy". Nature. 363 (6425): 140–142. Bibcode:1993Natur.363..140E. doi:10.1038/363140a0. ISSN 0028-0836.
- 1 2 Adams, Joshua J.; Hill, Gary J.; MacQueen, Phillip J. (2009-03-16). "B2 0902+34: A Collapsing Protogiant Elliptical Galaxy at z = 3.4". The Astrophysical Journal. 694 (1): 314–326. arXiv:0812.1333. Bibcode:2009ApJ...694..314A. doi:10.1088/0004-637x/694/1/314. ISSN 0004-637X.
- ↑ Rocca-Volmerange, B. (September 1988). "Age and star formation of the radio galaxy 0902+34 at redshift z = 3.395: constraints for primeval galaxies". The Messenger. 53: 26–29. Bibcode:1988Msngr..53...26R. ISSN 0722-6691.
- ↑ Fabian, A. C.; Crawford, C. S.; Iwasawa, K. (April 2002). "A Chandra observation of the distant radio galaxy B2 0902+343: a powerful obscured active galaxy". Monthly Notices of the Royal Astronomical Society. 331 (4): L57–L59. arXiv:astro-ph/0202449. Bibcode:2002MNRAS.331L..57F. doi:10.1046/j.1365-8711.2002.05452.x. ISSN 0035-8711.
- ↑ Reuland, Michiel; van Breugel, Wil; Röttgering, Huub; de Vries, Wim; Stanford, S. A.; Dey, Arjun; Lacy, Mark; Bland-Hawthorn, Joss; Dopita, Michael; Miley, George (August 2003). "Giant Lyα Nebulae Associated with High-Redshift Radio Galaxies". The Astrophysical Journal. 592 (2): 755–766. arXiv:astro-ph/0303637. Bibcode:2003ApJ...592..755R. doi:10.1086/375619. ISSN 0004-637X.
