Radio Galaxy Zoo: A search for hybrid morphology radio galaxies
Hybrid morphology radio sources (HyMoRS) are a rare type of radio galaxy that display different Fanaroff-Riley classes on opposite sides of their nuclei. To enhance the statistical analysis of HyMoRS, we embarked on a largescale search of these sources within the international citizen science projec...
| Main Authors: | , , , , , , , , , , , , , , , , |
|---|---|
| 格式: | Journal article |
| 出版: |
Institute of Physics
2017
|
| _version_ | 1826296348357427200 |
|---|---|
| author | Kapiñska, A Terentev, I Terentev, W Shabala, S Shabala, A Rudnick, L Storer, L Banfield, J Willett, K Willett, F Willett, C Willett, A Middelberg, E Norris, R Norris, K Seymour, N Simmons, B |
| author_facet | Kapiñska, A Terentev, I Terentev, W Shabala, S Shabala, A Rudnick, L Storer, L Banfield, J Willett, K Willett, F Willett, C Willett, A Middelberg, E Norris, R Norris, K Seymour, N Simmons, B |
| author_sort | Kapiñska, A |
| collection | OXFORD |
| description | Hybrid morphology radio sources (HyMoRS) are a rare type of radio galaxy that display different Fanaroff-Riley classes on opposite sides of their nuclei. To enhance the statistical analysis of HyMoRS, we embarked on a largescale search of these sources within the international citizen science project, Radio Galaxy Zoo (RGZ). Here, we present 25 new candidate hybrid morphology radio galaxies. Our selected candidates are moderate power radio galaxies (L median 4.7×10 24 WHz -1 sr -1 ) at redshifts 0.14 > z > 1.0. Hosts of nine candidates have spectroscopic observations, of which six are classified as quasars, one as high- A nd two as low-excitation galaxies. Two candidate HyMoRS are giant ( > 1 Mpc) radio galaxies, one resides at the center of a galaxy cluster, and one is hosted by a rare green bean galaxy. Although the origin of the hybrid morphology radio galaxies is still unclear, this type of radio source starts depicting itself as a rather diverse class. We discuss hybrid radio morphology formation in terms of the radio source environment (nurture) and intrinsically occurring phenomena (nature; activity cessation and amplification), showing that these peculiar radio galaxies can be formed by both mechanisms. While high angular resolution follow-up observations are still necessary to confirm our candidates, we demonstrate the efficacy of the RGZ in the pre-selection of these sources from all-sky radio surveys, and report the reliability of citizen scientists in identifying and classifying complex radio sources. |
| first_indexed | 2024-03-07T04:14:57Z |
| format | Journal article |
| id | oxford-uuid:c91d70a6-fd83-457c-b56c-526a73537df2 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T04:14:57Z |
| publishDate | 2017 |
| publisher | Institute of Physics |
| record_format | dspace |
| spelling | oxford-uuid:c91d70a6-fd83-457c-b56c-526a73537df22022-03-27T06:56:48ZRadio Galaxy Zoo: A search for hybrid morphology radio galaxiesJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:c91d70a6-fd83-457c-b56c-526a73537df2Symplectic Elements at OxfordInstitute of Physics2017Kapiñska, ATerentev, ITerentev, WShabala, SShabala, ARudnick, LStorer, LBanfield, JWillett, KWillett, FWillett, CWillett, AMiddelberg, ENorris, RNorris, KSeymour, NSimmons, BHybrid morphology radio sources (HyMoRS) are a rare type of radio galaxy that display different Fanaroff-Riley classes on opposite sides of their nuclei. To enhance the statistical analysis of HyMoRS, we embarked on a largescale search of these sources within the international citizen science project, Radio Galaxy Zoo (RGZ). Here, we present 25 new candidate hybrid morphology radio galaxies. Our selected candidates are moderate power radio galaxies (L median 4.7×10 24 WHz -1 sr -1 ) at redshifts 0.14 > z > 1.0. Hosts of nine candidates have spectroscopic observations, of which six are classified as quasars, one as high- A nd two as low-excitation galaxies. Two candidate HyMoRS are giant ( > 1 Mpc) radio galaxies, one resides at the center of a galaxy cluster, and one is hosted by a rare green bean galaxy. Although the origin of the hybrid morphology radio galaxies is still unclear, this type of radio source starts depicting itself as a rather diverse class. We discuss hybrid radio morphology formation in terms of the radio source environment (nurture) and intrinsically occurring phenomena (nature; activity cessation and amplification), showing that these peculiar radio galaxies can be formed by both mechanisms. While high angular resolution follow-up observations are still necessary to confirm our candidates, we demonstrate the efficacy of the RGZ in the pre-selection of these sources from all-sky radio surveys, and report the reliability of citizen scientists in identifying and classifying complex radio sources. |
| spellingShingle | Kapiñska, A Terentev, I Terentev, W Shabala, S Shabala, A Rudnick, L Storer, L Banfield, J Willett, K Willett, F Willett, C Willett, A Middelberg, E Norris, R Norris, K Seymour, N Simmons, B Radio Galaxy Zoo: A search for hybrid morphology radio galaxies |
| title | Radio Galaxy Zoo: A search for hybrid morphology radio galaxies |
| title_full | Radio Galaxy Zoo: A search for hybrid morphology radio galaxies |
| title_fullStr | Radio Galaxy Zoo: A search for hybrid morphology radio galaxies |
| title_full_unstemmed | Radio Galaxy Zoo: A search for hybrid morphology radio galaxies |
| title_short | Radio Galaxy Zoo: A search for hybrid morphology radio galaxies |
| title_sort | radio galaxy zoo a search for hybrid morphology radio galaxies |
| work_keys_str_mv | AT kapinskaa radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT terentevi radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT terentevw radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT shabalas radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT shabalaa radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT rudnickl radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT storerl radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT banfieldj radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT willettk radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT willettf radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT willettc radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT willetta radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT middelberge radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT norrisr radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT norrisk radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT seymourn radiogalaxyzooasearchforhybridmorphologyradiogalaxies AT simmonsb radiogalaxyzooasearchforhybridmorphologyradiogalaxies |