SWIFT J1626.6-5156 is not a high mass X-ray binary

Details SWIFT J1626.6-5156 is not a high mass X-ray binary SWIFT J1626.6-5156 is not a high mass X-ray binary

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..713....1r&link_type=abstract

The Astronomer's Telegram, #713

Astronomy and Astrophysics

Astronomy

9

Infra-Red, Optical, Request For Observations, Pulsars, Transients

Scientific paper

on behalf of E. Molinari, G. Chincarini, F.M. Zerbi, S. Covino, G. Tosti, P. Conconi, G. Cutispoto, L. Nicastro, E. Palazzi, F. Vitali, F. D'Alessio, E. Meurs, P. Goldoni and the REMIR/ROSS collaboration We report on infrared observations of the newly discovered transient X-ray pulsar SWIFT J1626.6-5156 (Palmer et al., ATEL #678, Markwardt & Swank, ATEL #679 and Campana et al., ATEL #688).

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