Astron. Astrophys. Suppl. Ser. 132
November(I) 1998

1998A&AS..132..305T – (Tables: J/A+AS/132/305)
Fifteen years monitoring of extragalactic radio sources at 22, 37 and 87 GHz.
Teraesranta H., Tornikoski M., Mujunen A., Karlamaa K., Valtonen T., Henelius N., Urpo S., Lainela M., Pursimo T., Nilsson K., Wiren S., Laehteenmaeki A., Korpi M., Rekola R., Heinaemaeki P., Hanski M., Nurmi P., Kokkonen K., Keinaenen P., Joutsamo O., Oksanen J., Pietilae H., Valtaoja E., Valtonen M., Koenoenen P.
1998A&AS..132..333B
Terzan 3 and IC 1276 (Palomar 7): Two metal-rich bulge globular clusters uncovered.
Barbuy B., Ortolani S., Bica E.
1998A&AS..132..341M – (Tables: J/A+AS/132/341)
Identification of selected sources from the ROSAT Galactic Plane Survey. I.
Motch C., Guillout P., Haberl F., Krautter J., Pakull M.W., Pietsch W., Reinsch K., Voges W., Zickgraf F.-J.
1998A&AS..132..361R – (Tables: J/A+AS/132/361)
Optical observations of eight X-ray selected BL Lacertae objects.
Raiteri C.M., Villata M., De Francesco G., Lanteri L., Cavallone M., Sobrito G.
1998A&AS..132..367B – (Tables: J/A+AS/132/367)
Physical parameters of the Algol system TZ Eridani from simultaneous analysis of Geneva 7-colour light curves.
Barblan F., Bartholdi P., North P., Burki G., Olson E.C.
1998A&AS..132..381M
Check on JPL DE405 using modern optical observations.
Morrison L.V., Evans D.W.
1998A&AS..132..387K
Results of the digital co-addition of thirteen Schmidt films of the Virgo cluster of galaxies.
Katsiyannis A.C., Kemp S.N., Berry D.S., Meaburn J.
1998A&AS..132..401U
A 1.4 GHz radio continuum and polarization survey at medium Galactic latitudes. I. Observation and reduction technique.
Uyaniker B., Fuerst E., Reich W., Reich P., Wielebinski R.
1998A&AS..132..413G
The gain-elevation correction of the IRAM 30-m telescope.
Greve A., Neri R., Sievers A.
1998A&AS..132..417W
Determination of orbital parameters of interacting galaxies using a genetic algorithm. Description of the method and application to artificial data.
Wahde M.
1998A&AS..132..431N
Construction of highly accurate models of rotating neutron stars - comparison of three different numerical schemes.
Nozawa T., Stergioulas N., Gourgoulhon E., Eriguchi Y.
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