From BCB issue no. 72 (June 2001) on, the editor-in-chief will change.
I am pleased to announce that
I like to express my sincere thanks to all past and current members of the
editorial team for their extensive efforts as contributing editors during
the past five years. Thanks to their excellent collaboration, it was a real
pleasure to compile this bibliography.
Horst Drechsel
ALL future issues of BCB will be distributed electronically, except in rare and unusual circumstances. Would ALL those receiving this hardcopy please contact the new editor in one of three ways:
Please note that the reasons are important; a simple statement of
preference for hardcopy will be ignored and TREATED AS LACK OF ANY
RESPONSE. PLEASE NOTE ALSO THAT IT WILL BE ASSUMED THAT THOSE WHO DO NOT
RESPOND AT ALL DO NOT WISH TO RECEIVE ANY FURTHER ISSUES OF THIS
BIBLIOGRAPHY.
For those who now receive BCB electronically, no action is necessary, since the current editor will provide his successor with a full email address list. But all recipients are responsible for keeping the editor informed about future address changes; these should be sent to the new editor, starting immediately.
The bibliographical entries for Individual Stars and Collections
of Data are categorized according to the following coding scheme:
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 | HMXB | high-mass X-ray binary | QPO | quasi-periodic oscillation |
BH | black hole | IP | intermediate polar | RV | radial velocity |
CB | close binary | LC | light curve | SB | spectroscopic binary |
CV | cataclysmic variable | LMXB | low-mass X-ray binary | WD | white dwarf |
EB | eclipsing binary | NS | neutron star | WR | Wolf-Rayet star |
Several entries of this issue use the abbreviation:
OAP -- Odessa Astronomical Publications
(issue of the Odessa Astronomical Observatory of the Odessa State University,
Ukraine), Astroprint Publishing Company, Ukraine