OBSERVATIONS

We have obtained new spectra for 11 FBS objects. The observations were carried out on November 25, 1998 and January 14-15, 1999 at the Byurakan Astrophysical Observatory (BAO) and at the Observatoire de Haute-Provence (OHP), respectively. The journal of observations is given in Table 1, together with relevant data.

**Table:** New spectra. Col. 1 gives the name, col. 2 the FBS number, col. 3 the original FBS classification, col. 4 the magnitude, cols. 5 and 6 the place and date of observation, col. 7 the galactic latitude, col. 8 the classification and col. 9 the redshift
	FBS #		mag		date	b		z
FBS0228+447	227	B2	15.5	BAO	25.11.98	-14.4	*
FBS0744+818	1055	B1e	16.4	OHP	14.01.99	29.1	*
FBS0747+729	966	N3e	15.8	BAO	25.11.98	30.4	*
FBS0929+733	876	B3e	16.3	BAO	25.11.98	37.2	*
FBS0944+713	878	B3e	18.6	OHP	14.01.99	39.3	*
FBS0950+664	785	N2	16.7	BAO	25.11.98	42.4	S1	0.172
FBS1049+803	1068	N1e	17.1	BAO	25.11.98	35.7	*
FBS1235+699	894	N1e	17.9	OHP	15.01.99	47.4	Q	0.521
FBS1324+448	322	B1	17.	OHP	15.01.99	71.1	Q	0.331
FBS1715+406	936	se	16.	OHP	18.01.99	34.5	G	0.029
FBS2308+425	418	B1	13.5	OHP	14.01.99	-16.3	*

Seven of the newly observed objects are stars, including FBS2308+425 (at b = -16.3 $^\circ$ ) which is associated with a ROSAT RASS (Voges et al. 1999) X-ray source (Table 2, Paper I).

FBS0950+664 (RXS J09540+6608) has been identified on an objective prism plate as an AGN (Bade et al. 1998); our spectrum shows it to be a Seyfert 1 at z = 0.172. Our new spectra of FBS1235+699 and FBS1324+448 confirm their redshift (z = 0.521 and 0.331 respectively). FBS1715+406 is Zw225.094 or MCG07.35.061, a 15.4 mag galaxy at z = 0.030 (Marzke et al. 1996); according to Abramian & Mickaelian (1994), it is an emission line galaxy; our spectrum shows that it is an absorption line galaxy, with a weak [Nii] $\lambda$ 6583 line in emission at z = 0.029.

**Figure:** Spectra of the four extragalactic objects in Table .
$\begin{figure} \begin{center} \resizebox {14cm}{!}{\includegraphics{areg_plot.eps}} \end{center}\end{figure}$