PSR B1902+04.1 , the SIMBAD biblio

PSR B1902+04.1 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST03:13:47

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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
2000ApJ...530L..93T 4 10 140 Formation of millisecond pulsars with heavy white dwarf companions : extreme mass transfer on subthermal timescales. TAURIS T.M., VAN DEN HEUVEL E.P.J. and SAVONIJE G.J.
2000ApJ...541..329T 43 37 On a theoretical interpretation of the period gap in binary millisecond pulsars. TAAM R.E., KING A.R. and RITTER H.
2000AAS...197.8313C 8 0 Intermediate-mass binary pulsars from the Parkes multibeam survey. CAMILO F., LYNE A.G., STAIRS I.H., et al.
2001A&A...376..165L 12 2 The residual orbital eccentricity in close binaries. An application to millisecond binary pulsars. LANZA A.F. and RODONO M.
2001ApJ...548L.187C 38   K                 8 52 Discovery of five binary radio pulsars. CAMILO F., LYNE A.G., MANCHESTER R.N., et al.
2001ApJ...553..801E 30 41 Recycled pulsars discovered at high radio frequency. EDWARDS R.T. and BAILES M.
2002ApJ...564..930L 37   K                 6 16 Formation of mildly recycled low-mass binary pulsars from intermediate-mass X-ray binaries. LI X.-D.
2002MNRAS.335..275M viz 123 168 The Parkes Multibeam Pulsar Survey - II. Discovery and timing of 120 pulsars. MORRIS D.J., HOBBS G., LYNE A.G., et al.
2004ApJ...605..759B viz 15       D               99 280 Multifrequency observations of radio pulse broadening and constraints on interstellar electron density microstructure. BHAT N.D.R., CORDES J.M., CAMILO F., et al.
2004Sci...304..547S 1 57 177 Pulsars in binary systems: probing binary stellar evolution and general relativity. STAIRS I.H.
2005A&A...439..635A 44 17 TeV gamma-ray observations of SS-433 and a survey of the surrounding field with the HEGRA IACT-System. AHARONIAN F., AKHPERJANIAN A., BEILICKE M., et al.
2007PhR...442....5B 53 16 Evolution and merging of binaries with compact objects. BETHE H.A., BROWN G.E. and LEE C.-H.
2010ApJ...715..335K 15       D               1 87 25 Millisecond pulsar ages: implications of binary evolution and a maximum spin limit. KIZILTAN B. and THORSETT S.E.
2012MNRAS.425.1601T 16       D               1 52 165 Formation of millisecond pulsars with CO white dwarf companions – II. Accretion, spin-up, true ages and comparison to MSPs with He white dwarf companions. TAURIS T.M., LANGER N. and KRAMER M.
2013MNRAS.432L..75C 16       D               1 18 2 Evolution of neutron star + He star binaries: an alternative evolutionary channel to intermediate-mass binary pulsars. CHEN W.-C. and LIU W.-M.
2014ApJ...785..119A viz 16       D               1 202 131 Gravitational waves from known pulsars: results from the initial detector era. AASI J., ABADIE J., ABBOTT B.P., et al.
2014MNRAS.441.3615L 16       D               1 18 1 Magnetic braking of Ap/Bp stars: an alternative formation mechanism of compact intermediate-mass binary pulsars. LIU W.-M. and CHEN W.-C.
2015ApJ...812...81L viz 16       D               1 174 83 Arecibo Pulsar survey using ALFA. IV. Mock spectrometer data analysis, survey sensitivity, and the discovery of 40 pulsars. LAZARUS P., BRAZIER A., HESSELS J.W.T., et al.
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.
2017MNRAS.464..237S 16       D               1 18 2 The implications of a companion enhanced wind on millisecond pulsar production. SMEDLEY S.L., TOUT C.A., FERRARIO L., et al.
2019ApJ...879...10A viz 17       D               1 225 87 Searches for gravitational waves from known pulsars at two harmonics in 2015-2017 LIGO data. ABBOTT B.P., ABBOTT R., ABBOTT T.D., et al.
2021ApJS..255....5A viz 17       D               1 977 ~ The CHIME pulsar project: system overview. AMIRI M., BANDURA K.M., BOYLE P.J., et al.
2022MNRAS.511.4669K 45           X         1 250 ~ Distances of galactic radio pulsars: first quadrant: -2° < l < 90° and -2° < b < 2°. KUTUKCU P., ANKAY A., YAZGAN E., et al.

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