J/A+AS/139/141 J/A+AS/139/141 Galaxies in the Perseus Cluster J Brunzendorf H Meusinger Astron. Astrophys. Suppl. Ser. 139 141 1999 1999A&AS..139..141B Clusters, galaxy Magnitudes Radial velocities Morphology galaxies: clusters: individual (A 426) galaxies: fundamental parameters galaxies: luminosity function A new catalogue of 660 galaxies within a field of about 10 square degrees in the Perseus cluster region is presented. The catalogue contains accurate positions, isophotal magnitudes, angular radii, position angles, radial velocities, morphological types, and detailed informations on morphological peculiarities. If available, cross identifications and radial velocities are also given. The catalogue is estimated to be complete to a 25mag isophotal B magnitude of about 18.

Sequence Running number in this catalogue --- Names Common names --- RAh Right ascension (J2000) h RAm Right ascension (J2000) min RAs Right ascension (J2000) s DE- Declination (sign) --- DEd Declination (J2000) deg DEm Declination (J2000) arcmin DEs Declination (J2000) arcsec Mag25 Apparent B magnitude within B25 mag/arcsec^2^ isophote Without corrections for Galactic foreground extinction and inclination. mag u_Mag25 Uncertainty flag for Mag25 Typical uncertainties of Mag25 are 0.1 to 0.2 mag. Larger uncertainties due to difficulties in the removal of foreground stars are marked by a colon --- SuBr Central B surface brightness mag u_SuBr Uncertainty flag for SuBr --- a25 Major axis of the B25 mag/arcsec^2^ isophote arcsec b25 Minor axis of the B25 mag/arcsec^2^ isophote arcsec PA Position angle, North to East deg REM Remark number about size or photometry 1: a25, b25, PA are difficult to estimate for the individual components of this merger system 2: Mag25, a25, b25, PA are related to the central knot; the outer ring has a radius of 27 arcsec --- HRV Heliocentric radial velocity km/s Mtype Morphological Type --- n_Mtype Note on morphology and/or environment The following symbols are used: IN: systems with signs of strong interaction in the form of bridges (br) and/or tails (ta) DIS: systems with signs of distortions, which can show one or several of the following features coded by a number: (1) peculiar spiral arms (2) three-armed spirals (3) M51 type (4) unusual dust absorption (5) elliptical galaxy with isophote twist (6) non-concentric core (7) loops/shells (8) jet-like structures (9) fuzzy structure in the outer regions (10) radial spikes CH(n): n systems (n>1) within a common halo PL: polar ring galaxies or related objects f*: estimation of morphology hampered by a nearby foreground star The strength of the morphological peculiarity is indicated (+ for strong, - for weak). --- Helmut Meusinger TLS Tautenburg 1999Jul19Helmut Meusinger <meus@obelix.tls-tautenburg.de> J_A+AS_139_141.xml