PSR J1836-2354A , the SIMBAD biblio

PSR J1836-2354A , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:11:17

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2011ApJ...734...89L 91   K   D     X         3 23 10 Six new recycled globular cluster pulsars discovered with the Green Bank telescope. LYNCH R.S., RANSOM S.M., FREIRE P.C.C., et al.
2011MNRAS.418..477B 91       D       C       2 132 31 Luminosities of recycled radio pulsars in globular clusters. BAGCHI M., LORIMER D.R. and CHENNAMANGALAM J.
2013A&A...551A..60W 38         O X         1 45 4 CV1 in the globular cluster M 22: confirming its nature through X-ray observations and optical spectroscopy. WEBB N.A. and SERVILLAT M.
2015BaltA..24..395M viz 16       D               1 619 2 Binary star DataBase: binaries discovered in non-optical bands. MALKOV O.Y., TESSEMA S.B. and KNIAZEV A.Y.
2017ApJ...835...29Y 17       D               1 301 678 A new electron-density model for estimation of pulsar and FRB distances. YAO J.M., MANCHESTER R.N. and WANG N.
2018MNRAS.480..692P 16       D               1 20 3 The minimum magnetic field of millisecond pulsars calculated according to accretion: application to the X-ray neutron star SAX J1808.4-3658 in a low-mass X-ray binary. PAN Y.Y., ZHANG C.M., SONG L.M., et al.
2019MNRAS.486.3992A 1933 T K A     X C       46 27 1 Search for multiwavelength emission from the binary millisecond pulsar
PSR
J1836-2354A in the globular cluster M22. 		AMATO R., D'AI A., DEL SANTO M., et al.
2019A&A...629A..92G 16       D               3 43 ~ Timing of PSR J2055+3829, an eclipsing black widow pulsar discovered with the Nancay Radio Telescope. GUILLEMOT L., OCTAU F., COGNARD I., et al.
2020MNRAS.492.5684H 41           X         1 107 ~ The X-ray emissivity of low-density stellar populations. HEINKE C.O., IVANOV M.G., KOCH E.W., et al.
2020MNRAS.495.3656G 16       D               1 27 19 Black widow evolution: magnetic braking by an ablated wind. GINZBURG S. and QUATAERT E.
2020MNRAS.496.4488H 41           X         1 277 ~ Counterparts of Far Eastern Guest Stars: Novae, supernovae, or something else? HOFFMANN S.M. and VOGT N.
2022MNRAS.511.5964Z viz 17       D               1 113 10 A census of X-ray millisecond pulsars in globular clusters. ZHAO J. and HEINKE C.O.
2023ApJ...944..225L 17       D               1 141 ~ A Comparison of Millisecond Pulsar Populations between Globular Clusters and the Galactic Field. LEE J., HUI C.Y., TAKATA J., et al.
2023ApJ...945...70Z 17       D               1 66 1 Likely Detection of γ-Ray Pulsations of PSR J1717+4308A in NGC 6341 and Implication of the γ-Ray Millisecond Pulsars in Globular Clusters. ZHANG P., XING Y., WANG Z., et al.
2023MNRAS.525.3963K 104       D     X         3 86 ~ A Gaia view of the optical and X-ray luminosities of compact binary millisecond pulsars. KOLJONEN K.I.I. and LINARES M.
2023ApJ...957...52T 17       D               2 16 ~ Probing the Solar Interior with Lensed Gravitational Waves from Known Pulsars. TAKAHASHI R., MORISAKI S. and SUYAMA T.
2023MNRAS.526.2736Z 17       D               1 80 ~ A Chandra X-ray study of millisecond pulsars in the globular cluster Omega Centauri: a correlation between spider pulsar companion mass and X-ray luminosity. ZHAO J. and HEINKE C.O.
2024ApJ...971..180Y 45           X         1 76 ~ A Multiwavelength Machine-learning Approach to Classifying X-Ray Sources in the Fields of Unidentified 4FGL-DR4 Sources. YANG H., HARE J. and KARGALTSEV O.
2024A&A...692A.187G 18       D               1 75 ~ Millisecond pulsars phenomenology under the light of graph theory. GARCIA C.R., ILLIANO G., TORRES D.F., et al.
2025ApJ...979..143K 19       D               1 123 ~ Unveiling Low-frequency Eclipses in Spider Millisecond Pulsars Using Wideband GMRT Observations. KUMARI S., BHATTACHARYYA B., KANSABANIK D., et al.
2025ApJ...992..116M 19       D               1 181 ~ Irradiated Pulsar Planets and Companions as 511 keV Positron Annihilation Line Sources. METZLER Z. and WADIASINGH Z.

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