a. | Photometry |
b. | Spectroscopy |
c. | Spectrophotometry |
d. | Polarimetry |
e. | Astrometry, interferometry |
f. | Times of minima |
g. | ![]() |
i. | Infrared data |
o. | Optical data |
p. | Photographic data |
r. | Radio data |
u. | Ultraviolet data |
v. | Visual estimates |
x. | X-ray data |
a. | Orbital elements |
b. | Absolute dimensions, masses |
c. | New or improved ephemeris, period variations |
d. | Apsidal motion |
e. | Physical properties of stellar atmospheres |
f. | Chemical abundances |
g. | Accretion disks and accretion phenomena |
a.
Catalogues
b.
Discoveries of new binaries and novae
c.
Identification of optical counterparts of X-ray, IR, or
radio sources
d.
Finding charts
a.
Abstract
b.
Addenda or errata
Abbreviations
AD | accretion disk | EB | eclipsing binary | RV | radial velocity |
BH | black hole | HMXB | high-mass X-ray binary | SB | spectroscopic binary |
CB | close binary | LMXB | low-mass X-ray binary | WD | white dwarf |
CV | cataclysmic variable | NS | neutron star | WR | Wolf-Rayet |
Acknowledgements
Dr. B.J. Carrigan and Dr. R. Häfner can no longer serve as contributing
editors due to other responsibilities. From BPN issue no. 65 on, their
review tasks were taken over by Dr. D.R. Faulkner and Dr. M. Wolf. I like to
thank the former team members for their excellent work and efforts, and
am looking forward to a pleasant collaboration with the new colleagues.
H. Drechsel