2006/09/30 by M. Falanga, Juri Poutanen, J. Poutanen +6
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Gamma-ray bursts and supernovae #Millisecond #Millisecond pulsar #Physics #Pulsar #Pulsars and Gravitational Waves Research #Spectral analysis #Spectroscopy #Transient (computer programming) #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066457
7 pages, 4 figures, accepted for publication in A&A
openalex publication_date 2007/01/11 · arxiv created 2007/01/13 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05
Aims.HETE J1900.1–2455 is the seventh known X-ray transient accreting millisecond pulsar and has been in outburst for more than one year. We compared the data on HETE J1900.1–2455 with other similar objects and made an attempt at deriving constraints on the physical processes responsible for a spectral formation.