Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.authorSzabo, Zsofia Marianna
dc.contributor.authorGong, Yan
dc.contributor.authorYang, Wenjin
dc.contributor.authorMenten, Karl M.
dc.contributor.authorBayandina, Olga S.
dc.contributor.authorCyganowski, Claudia Jane
dc.contributor.authorKóspál, Ágnes
dc.contributor.authorÁbrahám, Péter
dc.contributor.authorBeloche, Arnaud
dc.contributor.authorWyrowski, Friedrich
dc.date.accessioned2024-02-09T16:30:06Z
dc.date.available2024-02-09T16:30:06Z
dc.date.issued2024-02-07
dc.identifier292864733
dc.identifier2d041f96-20b1-4fc2-ad46-0a73a040fe8d
dc.identifier85185782567
dc.identifier.citationSzabo , 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/S1743921323003174en
dc.identifier.issn1743-9213
dc.identifier.otherORCID: /0000-0001-9830-3509/work/152898800
dc.identifier.urihttps://hdl.handle.net/10023/29205
dc.descriptionFunding: H2020 European Research Council - 716155.en
dc.description.abstractThe 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.extent3
dc.format.extent269760
dc.language.isoeng
dc.relation.ispartofProceedings of the International Astronomical Unionen
dc.subjectStars: pre-main sequenceen
dc.subjectStars: low massen
dc.subjectMasersen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleH2O masers and host environments of FU Orionis and EX Lupi type low-mass eruptive YSOsen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doi10.1017/S1743921323003174
dc.description.statusPeer revieweden


This item appears in the following Collection(s)

Show simple item record