Loading…
Extreme HBL-like behavior of Markarian 421 and its two-zone photohadronic interpretation
Markarian 421 is the nearest high-energy peaked blazar and also is the first extragalactic source to be detected in multi-TeV \(\gamma\)-rays. It has been observed in multiwavelength for exceptionally long period of time with dense monitoring and several major outbursts have been detected from this...
Saved in:
Published in: | arXiv.org 2021-04 |
---|---|
Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | |
container_end_page | |
container_issue | |
container_start_page | |
container_title | arXiv.org |
container_volume | |
creator | Sahu, Sarira López Fortín, Carlos E Isabel Abigail Valadez Polanco Rajpoot, Subhash |
description | Markarian 421 is the nearest high-energy peaked blazar and also is the first extragalactic source to be detected in multi-TeV \(\gamma\)-rays. It has been observed in multiwavelength for exceptionally long period of time with dense monitoring and several major outbursts have been detected from this source. In March 2010, the source was in a high state of activity and was observed in multiwavelength by various telescopes for 13 consecutive days. During this period the position of the synchrotron peak was found to be above \(10^{17}\) Hz and also the position of the second peak was shifted towards higher energy, a signature of extreme HBL-like behavior. We observed that the standard photohadronic model is inadequate to explain the observed spectra. However, a recently proposed two-zone photohadronic model explains very well the GeV-TeV flaring events observed by both MAGIC and VERITAS telescopes. From the observation of the highest energy \(\gamma\)-ray event on MJD 55266 we also estimated the minimum bulk Lorentz factor. |
doi_str_mv | 10.48550/arxiv.2104.11999 |
format | article |
fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2518862294</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2518862294</sourcerecordid><originalsourceid>FETCH-LOGICAL-a524-614571f19d512c97ba23b3e3c688d0c30042c7468fcba818f530ffaf6f7e01b43</originalsourceid><addsrcrecordid>eNotzUFLwzAYgOEgCI65H-At4Lk135ekTY86phtMvOzgbXxtE5ZtJjXN5vDXK-jpvT0vY3cgSmW0Fg-ULv5cIghVAjRNc8UmKCUURiHesNk47oUQWNWotZyw98UlJ_th-fJpXRz9wfLW7ujsY-LR8VdKB0qeAlcInELPfR55_orFdwyWD7uY4476FIPvuA_ZpiHZTNnHcMuuHR1HO_vvlG2eF5v5sli_vazmj-uCNKqiAqVrcND0GrBr6pZQttLKrjKmF50UQmFXq8q4riUDxmkpnCNXudoKaJWcsvs_dkjx82THvN3HUwq_xy1qMKZCbJT8AV0bUsg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2518862294</pqid></control><display><type>article</type><title>Extreme HBL-like behavior of Markarian 421 and its two-zone photohadronic interpretation</title><source>Publicly Available Content Database</source><creator>Sahu, Sarira ; López Fortín, Carlos E ; Isabel Abigail Valadez Polanco ; Rajpoot, Subhash</creator><creatorcontrib>Sahu, Sarira ; López Fortín, Carlos E ; Isabel Abigail Valadez Polanco ; Rajpoot, Subhash</creatorcontrib><description>Markarian 421 is the nearest high-energy peaked blazar and also is the first extragalactic source to be detected in multi-TeV \(\gamma\)-rays. It has been observed in multiwavelength for exceptionally long period of time with dense monitoring and several major outbursts have been detected from this source. In March 2010, the source was in a high state of activity and was observed in multiwavelength by various telescopes for 13 consecutive days. During this period the position of the synchrotron peak was found to be above \(10^{17}\) Hz and also the position of the second peak was shifted towards higher energy, a signature of extreme HBL-like behavior. We observed that the standard photohadronic model is inadequate to explain the observed spectra. However, a recently proposed two-zone photohadronic model explains very well the GeV-TeV flaring events observed by both MAGIC and VERITAS telescopes. From the observation of the highest energy \(\gamma\)-ray event on MJD 55266 we also estimated the minimum bulk Lorentz factor.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2104.11999</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Gamma rays ; Lorentz factor ; Outbursts ; Synchrotrons ; Telescopes</subject><ispartof>arXiv.org, 2021-04</ispartof><rights>2021. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2518862294?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>778,782,25740,27912,36999,44577</link.rule.ids></links><search><creatorcontrib>Sahu, Sarira</creatorcontrib><creatorcontrib>López Fortín, Carlos E</creatorcontrib><creatorcontrib>Isabel Abigail Valadez Polanco</creatorcontrib><creatorcontrib>Rajpoot, Subhash</creatorcontrib><title>Extreme HBL-like behavior of Markarian 421 and its two-zone photohadronic interpretation</title><title>arXiv.org</title><description>Markarian 421 is the nearest high-energy peaked blazar and also is the first extragalactic source to be detected in multi-TeV \(\gamma\)-rays. It has been observed in multiwavelength for exceptionally long period of time with dense monitoring and several major outbursts have been detected from this source. In March 2010, the source was in a high state of activity and was observed in multiwavelength by various telescopes for 13 consecutive days. During this period the position of the synchrotron peak was found to be above \(10^{17}\) Hz and also the position of the second peak was shifted towards higher energy, a signature of extreme HBL-like behavior. We observed that the standard photohadronic model is inadequate to explain the observed spectra. However, a recently proposed two-zone photohadronic model explains very well the GeV-TeV flaring events observed by both MAGIC and VERITAS telescopes. From the observation of the highest energy \(\gamma\)-ray event on MJD 55266 we also estimated the minimum bulk Lorentz factor.</description><subject>Gamma rays</subject><subject>Lorentz factor</subject><subject>Outbursts</subject><subject>Synchrotrons</subject><subject>Telescopes</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotzUFLwzAYgOEgCI65H-At4Lk135ekTY86phtMvOzgbXxtE5ZtJjXN5vDXK-jpvT0vY3cgSmW0Fg-ULv5cIghVAjRNc8UmKCUURiHesNk47oUQWNWotZyw98UlJ_th-fJpXRz9wfLW7ujsY-LR8VdKB0qeAlcInELPfR55_orFdwyWD7uY4476FIPvuA_ZpiHZTNnHcMuuHR1HO_vvlG2eF5v5sli_vazmj-uCNKqiAqVrcND0GrBr6pZQttLKrjKmF50UQmFXq8q4riUDxmkpnCNXudoKaJWcsvs_dkjx82THvN3HUwq_xy1qMKZCbJT8AV0bUsg</recordid><startdate>20210424</startdate><enddate>20210424</enddate><creator>Sahu, Sarira</creator><creator>López Fortín, Carlos E</creator><creator>Isabel Abigail Valadez Polanco</creator><creator>Rajpoot, Subhash</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20210424</creationdate><title>Extreme HBL-like behavior of Markarian 421 and its two-zone photohadronic interpretation</title><author>Sahu, Sarira ; López Fortín, Carlos E ; Isabel Abigail Valadez Polanco ; Rajpoot, Subhash</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a524-614571f19d512c97ba23b3e3c688d0c30042c7468fcba818f530ffaf6f7e01b43</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Gamma rays</topic><topic>Lorentz factor</topic><topic>Outbursts</topic><topic>Synchrotrons</topic><topic>Telescopes</topic><toplevel>online_resources</toplevel><creatorcontrib>Sahu, Sarira</creatorcontrib><creatorcontrib>López Fortín, Carlos E</creatorcontrib><creatorcontrib>Isabel Abigail Valadez Polanco</creatorcontrib><creatorcontrib>Rajpoot, Subhash</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Databases</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sahu, Sarira</au><au>López Fortín, Carlos E</au><au>Isabel Abigail Valadez Polanco</au><au>Rajpoot, Subhash</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Extreme HBL-like behavior of Markarian 421 and its two-zone photohadronic interpretation</atitle><jtitle>arXiv.org</jtitle><date>2021-04-24</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>Markarian 421 is the nearest high-energy peaked blazar and also is the first extragalactic source to be detected in multi-TeV \(\gamma\)-rays. It has been observed in multiwavelength for exceptionally long period of time with dense monitoring and several major outbursts have been detected from this source. In March 2010, the source was in a high state of activity and was observed in multiwavelength by various telescopes for 13 consecutive days. During this period the position of the synchrotron peak was found to be above \(10^{17}\) Hz and also the position of the second peak was shifted towards higher energy, a signature of extreme HBL-like behavior. We observed that the standard photohadronic model is inadequate to explain the observed spectra. However, a recently proposed two-zone photohadronic model explains very well the GeV-TeV flaring events observed by both MAGIC and VERITAS telescopes. From the observation of the highest energy \(\gamma\)-ray event on MJD 55266 we also estimated the minimum bulk Lorentz factor.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2104.11999</doi><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | EISSN: 2331-8422 |
ispartof | arXiv.org, 2021-04 |
issn | 2331-8422 |
language | eng |
recordid | cdi_proquest_journals_2518862294 |
source | Publicly Available Content Database |
subjects | Gamma rays Lorentz factor Outbursts Synchrotrons Telescopes |
title | Extreme HBL-like behavior of Markarian 421 and its two-zone photohadronic interpretation |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-15T17%3A34%3A04IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Extreme%20HBL-like%20behavior%20of%20Markarian%20421%20and%20its%20two-zone%20photohadronic%20interpretation&rft.jtitle=arXiv.org&rft.au=Sahu,%20Sarira&rft.date=2021-04-24&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2104.11999&rft_dat=%3Cproquest%3E2518862294%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a524-614571f19d512c97ba23b3e3c688d0c30042c7468fcba818f530ffaf6f7e01b43%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2518862294&rft_id=info:pmid/&rfr_iscdi=true |