Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes

Context. In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV γ-ray emission from five novae. The GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. In this case it is expected that protons in the same conditions...

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Authors: MAGIC Collaboration; Marcote Martin, Benito; Munar i Adrover, Pere; Paredes i Poy, Josep Maria; Paredes Fortuny, Xavier; Ribó Gomis, Marc; Zanin, Roberta
Format: Article
Status:Accepted version
Publication date:2015
Country:España
Institution:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repository:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/69532
Online Access:https://hdl.handle.net/2445/69532
Access Level:Open access
Keyword:Estels binaris de raigs X
Noves (Estels)
Raigs gamma
X-ray binaries
New stars
Gamma rays
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author MAGIC Collaboration
author2 Marcote Martin, Benito
Munar i Adrover, Pere
Paredes i Poy, Josep Maria
Paredes Fortuny, Xavier
Ribó Gomis, Marc
Zanin, Roberta
author2_role author
author
author
author
author
author
author_browse MAGIC Collaboration
Marcote Martin, Benito
Munar i Adrover, Pere
Paredes Fortuny, Xavier
Paredes i Poy, Josep Maria
Ribó Gomis, Marc
Zanin, Roberta
author_facet MAGIC Collaboration
Marcote Martin, Benito
Munar i Adrover, Pere
Paredes i Poy, Josep Maria
Paredes Fortuny, Xavier
Ribó Gomis, Marc
Zanin, Roberta
author_role author
collection Recercat. Dipósit de la Recerca de Catalunya
description Context. In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV γ-ray emission from five novae. The GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. In this case it is expected that protons in the same conditions can be accelerated to much higher energies. Consequently they may produce a second component in the γ-ray spectrum at TeV energies. Aims: We aim to explore the very high-energy domain to search for γ-ray emission above 50 GeV and to shed light on the acceleration process of leptons and hadrons in nova explosions. Methods: We have performed observations, with the MAGIC telescopes of the classical nova V339 Del shortly after the 2013 outburst; optical and subsequent GeV γ-ray detections triggered the MAGIC observations. We also briefly report on VHE observations of the symbiotic nova YY Her and the dwarf nova ASASSN-13ax. We complement the TeV MAGIC observations with the analysis of contemporaneous Fermi-LAT data of the sources. The TeV and GeV observations are compared in order to evaluate the acceleration parameters for leptons and hadrons. Results: No significant TeV emission was found from the studied sources. We computed upper limits on the spectrum and night-by-night flux. The combined GeV and TeV observations of V339 Del limit the ratio of proton to electron luminosities to Lp ≲ 0.15 Le.
eu_rights_str_mv openAccess
format article
id ES_784a6aa8cdcfddc3de7b6089eb8b7bd0
institution Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
instname_str Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
network_acronym_str ES
network_name_str España
oai_identifier_str oai:recercat.cat:2445/69532
publishDate 2015
publishDateSort 2015
publisher Springer Verlag
publisherStr Springer Verlag
reponame_str Recercat. Dipósit de la Recerca de Catalunya
spelling Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes MAGIC Collaboration Marcote Martin, Benito Munar i Adrover, Pere Paredes i Poy, Josep Maria Paredes Fortuny, Xavier Ribó Gomis, Marc Zanin, Roberta Estels binaris de raigs X Noves (Estels) Raigs gamma X-ray binaries New stars Gamma rays Context. In the last five years the Fermi Large Area Telescope (LAT) instrument detected GeV γ-ray emission from five novae. The GeV emission can be interpreted in terms of an inverse Compton process of electrons accelerated in a shock. In this case it is expected that protons in the same conditions can be accelerated to much higher energies. Consequently they may produce a second component in the γ-ray spectrum at TeV energies. Aims: We aim to explore the very high-energy domain to search for γ-ray emission above 50 GeV and to shed light on the acceleration process of leptons and hadrons in nova explosions. Methods: We have performed observations, with the MAGIC telescopes of the classical nova V339 Del shortly after the 2013 outburst; optical and subsequent GeV γ-ray detections triggered the MAGIC observations. We also briefly report on VHE observations of the symbiotic nova YY Her and the dwarf nova ASASSN-13ax. We complement the TeV MAGIC observations with the analysis of contemporaneous Fermi-LAT data of the sources. The TeV and GeV observations are compared in order to evaluate the acceleration parameters for leptons and hadrons. Results: No significant TeV emission was found from the studied sources. We computed upper limits on the spectrum and night-by-night flux. The combined GeV and TeV observations of V339 Del limit the ratio of proton to electron luminosities to Lp ≲ 0.15 Le. Springer Verlag https://hdl.handle.net/2445/69532
spellingShingle Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
MAGIC Collaboration
Estels binaris de raigs X
Noves (Estels)
Raigs gamma
X-ray binaries
New stars
Gamma rays
status_str acceptedVersion
title Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
title_full Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
title_fullStr Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
title_full_unstemmed Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
title_short Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
title_sort Very high-energy γ-ray observations of novae and dwarf novae with the MAGIC telescopes
topic Estels binaris de raigs X
Noves (Estels)
Raigs gamma
X-ray binaries
New stars
Gamma rays
topic_facet Estels binaris de raigs X
Noves (Estels)
Raigs gamma
X-ray binaries
New stars
Gamma rays
url https://hdl.handle.net/2445/69532