Atti Del v Congresso Internazionale Di Filosofia 1925
DOI: 10.5840/wcp519251
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Relazione del Segretario Generale del V Congresso Internazionale di Filosofia

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“…There are far fewer confusing HII region sources at larger radius in the disk. Other high-velocity sources are pulsar wind nebulae (Gaensler 2005), hyper-velocity stars (Brown et al 2006) and runaway stars (del Valle & Romero 2012;del Valle et al 2013). The first type can be distinguished by observing the pulsar as well as its X-ray emission.…”
Section: Observational Signatures and Detectabilitymentioning
confidence: 99%
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“…There are far fewer confusing HII region sources at larger radius in the disk. Other high-velocity sources are pulsar wind nebulae (Gaensler 2005), hyper-velocity stars (Brown et al 2006) and runaway stars (del Valle & Romero 2012;del Valle et al 2013). The first type can be distinguished by observing the pulsar as well as its X-ray emission.…”
Section: Observational Signatures and Detectabilitymentioning
confidence: 99%
“…The first type can be distinguished by observing the pulsar as well as its X-ray emission. The last two types produce less synchrotron radiation (del Valle & Romero 2012;del Valle et al 2013), and thus can be distinguished as well. Globular clusters crossing the MW disk produce another class of contaminants.…”
Section: Observational Signatures and Detectabilitymentioning
confidence: 99%