Is there a dichotomy in the radio loudness distribution of quasars?
العنوان: | Is there a dichotomy in the radio loudness distribution of quasars? |
---|---|
المؤلفون: | Luigi Danese, Annalisa Celotti, Michele Cirasuolo, Manuela Magliocchetti |
المصدر: | Monthly Notices of the Royal Astronomical Society. 346:447-455 |
بيانات النشر: | Oxford University Press (OUP), 2003. |
سنة النشر: | 2003 |
مصطلحات موضوعية: | Physics, Jet (fluid), Accretion (meteorology), Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Astronomy and Astrophysics, Quasar, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Loudness, Luminosity, Space and Planetary Science, QUIET, Radiative transfer |
الوصف: | We present a new approach to tackle the issue of radio loudness in quasars. We constrain a (simple) prescription for the intrinsic distribution of radio-to-optical ratios by comparing properties of Monte Carlo simulated samples with those of observed optically selected quasars. We find strong evidence for a dependence of the radio luminosity on the optical one, even though with a large scatter. The dependence of the fraction of radio loud quasars on apparent and absolute optical magnitudes results in a selection effect related to the radio and optical limits of current surveys. The intrinsic distribution of the radio-to-optical ratios shows a peak at $R^*_{1.4} \sim 0.3$, with only $\simlt 5$ per cent of objects being included in a high $R^*_{1.4}$ tail which identifies the radio loud regime. No lack or deficit of sources -- but only a steep transition region -- is present between the radio loud and radio quiet populations at any $R^*_{1.4}$. We briefly discuss possible origins for this behaviour (e.g. absence of jets in radio quiet sources, large range of radiative radio efficiency, different life-times for the accretion and jet ejection phenomena, ...). |
تدمد: | 0035-8711 |
DOI: | 10.1046/j.1365-2966.2003.07105.x |
URL الوصول: | https://explore.openaire.eu/search/publication?articleId=doi_________::8e1e14d9757e41e41b0b38ec5b267c14 https://doi.org/10.1046/j.1365-2966.2003.07105.x |
Rights: | OPEN |
رقم الانضمام: | edsair.doi...........8e1e14d9757e41e41b0b38ec5b267c14 |
قاعدة البيانات: | OpenAIRE |
ResultId |
1 |
---|---|
Header |
edsair OpenAIRE edsair.doi...........8e1e14d9757e41e41b0b38ec5b267c14 784 3 unknown 784.149719238281 |
PLink |
https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi...........8e1e14d9757e41e41b0b38ec5b267c14&custid=s6537998&authtype=sso |
FullText |
Array
(
[Availability] => 0
)
Array ( [0] => Array ( [Url] => https://explore.openaire.eu/search/publication?articleId=doi_________::8e1e14d9757e41e41b0b38ec5b267c14# [Name] => EDS - OpenAIRE [Category] => fullText [Text] => View record in OpenAIRE [MouseOverText] => View record in OpenAIRE ) ) |
Items |
Array
(
[Name] => Title
[Label] => Title
[Group] => Ti
[Data] => Is there a dichotomy in the radio loudness distribution of quasars?
)
Array ( [Name] => Author [Label] => Authors [Group] => Au [Data] => <searchLink fieldCode="AR" term="%22Luigi+Danese%22">Luigi Danese</searchLink><br /><searchLink fieldCode="AR" term="%22Annalisa+Celotti%22">Annalisa Celotti</searchLink><br /><searchLink fieldCode="AR" term="%22Michele+Cirasuolo%22">Michele Cirasuolo</searchLink><br /><searchLink fieldCode="AR" term="%22Manuela+Magliocchetti%22">Manuela Magliocchetti</searchLink> ) Array ( [Name] => TitleSource [Label] => Source [Group] => Src [Data] => <i>Monthly Notices of the Royal Astronomical Society</i>. 346:447-455 ) Array ( [Name] => Publisher [Label] => Publisher Information [Group] => PubInfo [Data] => Oxford University Press (OUP), 2003. ) Array ( [Name] => DatePubCY [Label] => Publication Year [Group] => Date [Data] => 2003 ) Array ( [Name] => Subject [Label] => Subject Terms [Group] => Su [Data] => <searchLink fieldCode="DE" term="%22Physics%22">Physics</searchLink><br /><searchLink fieldCode="DE" term="%22Jet+%28fluid%29%22">Jet (fluid)</searchLink><br /><searchLink fieldCode="DE" term="%22Accretion+%28meteorology%29%22">Accretion (meteorology)</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysics%3A%3AHigh+Energy+Astrophysical+Phenomena%22">Astrophysics::High Energy Astrophysical Phenomena</searchLink><br /><searchLink fieldCode="DE" term="%22Monte+Carlo+method%22">Monte Carlo method</searchLink><br /><searchLink fieldCode="DE" term="%22Astronomy+and+Astrophysics%22">Astronomy and Astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Quasar%22">Quasar</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysics%3A%3ACosmology+and+Extragalactic+Astrophysics%22">Astrophysics::Cosmology and Extragalactic Astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Astrophysics%22">Astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Loudness%22">Loudness</searchLink><br /><searchLink fieldCode="DE" term="%22Luminosity%22">Luminosity</searchLink><br /><searchLink fieldCode="DE" term="%22Space+and+Planetary+Science%22">Space and Planetary Science</searchLink><br /><searchLink fieldCode="DE" term="%22QUIET%22">QUIET</searchLink><br /><searchLink fieldCode="DE" term="%22Radiative+transfer%22">Radiative transfer</searchLink> ) Array ( [Name] => Abstract [Label] => Description [Group] => Ab [Data] => We present a new approach to tackle the issue of radio loudness in quasars. We constrain a (simple) prescription for the intrinsic distribution of radio-to-optical ratios by comparing properties of Monte Carlo simulated samples with those of observed optically selected quasars. We find strong evidence for a dependence of the radio luminosity on the optical one, even though with a large scatter. The dependence of the fraction of radio loud quasars on apparent and absolute optical magnitudes results in a selection effect related to the radio and optical limits of current surveys. The intrinsic distribution of the radio-to-optical ratios shows a peak at $R^*_{1.4} \sim 0.3$, with only $\simlt 5$ per cent of objects being included in a high $R^*_{1.4}$ tail which identifies the radio loud regime. No lack or deficit of sources -- but only a steep transition region -- is present between the radio loud and radio quiet populations at any $R^*_{1.4}$. We briefly discuss possible origins for this behaviour (e.g. absence of jets in radio quiet sources, large range of radiative radio efficiency, different life-times for the accretion and jet ejection phenomena, ...). ) Array ( [Name] => ISSN [Label] => ISSN [Group] => ISSN [Data] => 0035-8711 ) Array ( [Name] => DOI [Label] => DOI [Group] => ID [Data] => 10.1046/j.1365-2966.2003.07105.x ) Array ( [Name] => URL [Label] => Access URL [Group] => URL [Data] => <link linkTarget="URL" linkTerm="https://explore.openaire.eu/search/publication?articleId=doi_________::8e1e14d9757e41e41b0b38ec5b267c14" linkWindow="_blank">https://explore.openaire.eu/search/publication?articleId=doi_________::8e1e14d9757e41e41b0b38ec5b267c14</link><br /><link linkTarget="URL" linkTerm="https://doi.org/10.1046/j.1365-2966.2003.07105.x" linkWindow="_blank">https://doi.org/10.1046/j.1365-2966.2003.07105.x</link> ) Array ( [Name] => Copyright [Label] => Rights [Group] => Cpyrght [Data] => OPEN ) Array ( [Name] => AN [Label] => Accession Number [Group] => ID [Data] => edsair.doi...........8e1e14d9757e41e41b0b38ec5b267c14 ) |
RecordInfo |
Array
(
[BibEntity] => Array
(
[Identifiers] => Array
(
[0] => Array
(
[Type] => doi
[Value] => 10.1046/j.1365-2966.2003.07105.x
)
)
[Languages] => Array
(
[0] => Array
(
[Text] => Undetermined
)
)
[PhysicalDescription] => Array
(
[Pagination] => Array
(
[PageCount] => 9
[StartPage] => 447
)
)
[Subjects] => Array
(
[0] => Array
(
[SubjectFull] => Physics
[Type] => general
)
[1] => Array
(
[SubjectFull] => Jet (fluid)
[Type] => general
)
[2] => Array
(
[SubjectFull] => Accretion (meteorology)
[Type] => general
)
[3] => Array
(
[SubjectFull] => Astrophysics::High Energy Astrophysical Phenomena
[Type] => general
)
[4] => Array
(
[SubjectFull] => Monte Carlo method
[Type] => general
)
[5] => Array
(
[SubjectFull] => Astronomy and Astrophysics
[Type] => general
)
[6] => Array
(
[SubjectFull] => Quasar
[Type] => general
)
[7] => Array
(
[SubjectFull] => Astrophysics::Cosmology and Extragalactic Astrophysics
[Type] => general
)
[8] => Array
(
[SubjectFull] => Astrophysics
[Type] => general
)
[9] => Array
(
[SubjectFull] => Loudness
[Type] => general
)
[10] => Array
(
[SubjectFull] => Luminosity
[Type] => general
)
[11] => Array
(
[SubjectFull] => Space and Planetary Science
[Type] => general
)
[12] => Array
(
[SubjectFull] => QUIET
[Type] => general
)
[13] => Array
(
[SubjectFull] => Radiative transfer
[Type] => general
)
)
[Titles] => Array
(
[0] => Array
(
[TitleFull] => Is there a dichotomy in the radio loudness distribution of quasars?
[Type] => main
)
)
)
[BibRelationships] => Array
(
[HasContributorRelationships] => Array
(
[0] => Array
(
[PersonEntity] => Array
(
[Name] => Array
(
[NameFull] => Luigi Danese
)
)
)
[1] => Array
(
[PersonEntity] => Array
(
[Name] => Array
(
[NameFull] => Annalisa Celotti
)
)
)
[2] => Array
(
[PersonEntity] => Array
(
[Name] => Array
(
[NameFull] => Michele Cirasuolo
)
)
)
[3] => Array
(
[PersonEntity] => Array
(
[Name] => Array
(
[NameFull] => Manuela Magliocchetti
)
)
)
)
[IsPartOfRelationships] => Array
(
[0] => Array
(
[BibEntity] => Array
(
[Dates] => Array
(
[0] => Array
(
[D] => 19
[M] => 11
[Type] => published
[Y] => 2003
)
)
[Identifiers] => Array
(
[0] => Array
(
[Type] => issn-print
[Value] => 00358711
)
[1] => Array
(
[Type] => issn-locals
[Value] => edsair
)
[2] => Array
(
[Type] => issn-locals
[Value] => edsairFT
)
)
[Numbering] => Array
(
[0] => Array
(
[Type] => volume
[Value] => 346
)
)
[Titles] => Array
(
[0] => Array
(
[TitleFull] => Monthly Notices of the Royal Astronomical Society
[Type] => main
)
)
)
)
)
)
)
|
IllustrationInfo |