Observability of Single Neutron Stars at SRG/eROSITA

dc.contributor.author	Khokhryakova A.D.
dc.contributor.author	Biryukov A.V.
dc.contributor.author	Popov S.B.
dc.date.accessioned	2022-02-09T20:35:35Z
dc.date.available	2022-02-09T20:35:35Z
dc.date.issued	2021
dc.identifier.issn	1063-7729
dc.identifier.uri	https://dspace.kpfu.ru/xmlui/handle/net/169260
dc.description.abstract	Abstract: A four-year sky survey with the use of the eROSITA telescope on board the Spektr-RG observatory with focusing optics will provide the best coverage in the soft (0.5–2 keV) and standard (2–10 keV) X-ray ranges, both in terms of sensitivity and angular resolution. We have investigated the possibility of detecting various types of single neutron stars using eROSITA. Among the already known objects, eROSITA will be able to detect more than 160 pulsars, 21 magnetars, 7 central compact objects, all seven sources of the Magnificent Seven, and two other X-ray single neutron stars during the four-year mission. In addition, eROSITA is expected to be able to detect accreting single neutron stars, as well as discover new cooling neutron stars and magnetars.
dc.relation.ispartofseries	Astronomy Reports
dc.subject	neutron stars
dc.subject	pulsars
dc.subject	X-ray astronomy
dc.subject	X-ray observations
dc.title	Observability of Single Neutron Stars at SRG/eROSITA
dc.type	Article
dc.relation.ispartofseries-issue	7
dc.relation.ispartofseries-volume	65
dc.collection	Публикации сотрудников КФУ
dc.relation.startpage	615
dc.source.id	SCOPUS10637729-2021-65-7-SID85113657603

Файлы в этом документе

Имя: SCOPUS10637729-20 ...

Размер: 32.60Kb

Формат: PDF

Публикации сотрудников КФУ Scopus [24551]
Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.