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H2O masers and host environments of FU Orionis and EX Lupi type low-mass eruptive YSOs
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dc.contributor.author | Szabo, Zsofia Marianna | |
dc.contributor.author | Gong, Yan | |
dc.contributor.author | Yang, Wenjin | |
dc.contributor.author | Menten, Karl M. | |
dc.contributor.author | Bayandina, Olga S. | |
dc.contributor.author | Cyganowski, Claudia Jane | |
dc.contributor.author | Kóspál, Ágnes | |
dc.contributor.author | Ábrahám, Péter | |
dc.contributor.author | Beloche, Arnaud | |
dc.contributor.author | Wyrowski, Friedrich | |
dc.date.accessioned | 2024-02-09T16:30:06Z | |
dc.date.available | 2024-02-09T16:30:06Z | |
dc.date.issued | 2024-02-07 | |
dc.identifier | 292864733 | |
dc.identifier | 2d041f96-20b1-4fc2-ad46-0a73a040fe8d | |
dc.identifier | 85185782567 | |
dc.identifier.citation | Szabo , Z M , Gong , Y , Yang , W , Menten , K M , Bayandina , O S , Cyganowski , C J , Kóspál , Á , Ábrahám , P , Beloche , A & Wyrowski , F 2024 , ' H 2 O masers and host environments of FU Orionis and EX Lupi type low-mass eruptive YSOs ' , Proceedings of the International Astronomical Union , vol. 18 , no. S380 , pp. 246-248 . https://doi.org/10.1017/S1743921323003174 | en |
dc.identifier.issn | 1743-9213 | |
dc.identifier.other | ORCID: /0000-0001-9830-3509/work/152898800 | |
dc.identifier.uri | https://hdl.handle.net/10023/29205 | |
dc.description | Funding: H2020 European Research Council - 716155. | en |
dc.description.abstract | The FU Orionis (FUor) and EX Lupi (EXor) type objects are rare pre-main sequence low-mass stars undergoing accretion outbursts. Maser emission is widespread and is a powerful probe of mass accretion and ejection on small scales in star forming region. However, very little is known about the overall prevalence of water masers towards FUors/Exors. We present results from our survey using the Effelsberg 100-m telescope to observe the largest sample of FUors and EXors, plus additional Gaia alerted sources (with the potential nature of being eruptive stars), a total of 51 targets, observing the 22.2 GHz H2O maser, while simultaneously covering the NH3 23 GHz. | |
dc.format.extent | 3 | |
dc.format.extent | 269760 | |
dc.language.iso | eng | |
dc.relation.ispartof | Proceedings of the International Astronomical Union | en |
dc.subject | Stars: pre-main sequence | en |
dc.subject | Stars: low mass | en |
dc.subject | Masers | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | 3rd-NDAS | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | H2O masers and host environments of FU Orionis and EX Lupi type low-mass eruptive YSOs | en |
dc.type | Journal article | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | 10.1017/S1743921323003174 | |
dc.description.status | Peer reviewed | en |
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