7096 VII/96 Catalog of morphological properties of Abell clusters M F Struble H J Rood Astrophys. J. Suppl. Ser. 63 555 1987 1987ApJS...63..555S Clusters, galaxy Morphology galaxies: clusters: general galaxies: distances and redshifts galaxies: structure A catalog is presented which contains Rood-Sastry (1971, hereafter RS) morphological types for all 2712 Abell clusters.

Abell Abell cluster identification --- n_Abell An '*' indicates that the cluster is not in Abell's (1980) statistical sample --- Dist Distance class as given by Abell (1980) --- nGal Abell's (1980) number count of galaxies --- Radius Radius of the circular observation window which our data were obtained (1mm=67.14") mm RS1 Basic RS type number=1 Basic RS type: cD, B, L, C, F or I --- RS2 Subsidiary property of RS type number=2 Appendage or subscript which indicates a subsidiary property : p=peculiar cD galaxy n=multiple nucleus cD galaxy s=satellite of a cD galaxy b=connected supergiant binary galaxy within a B-type cluster p=peculiarity associated with a supergiant binary galaxy or the B cluster itself a=arc shape of the line of galaxies defining an L-type cluster c=clumpy s=smooth I-type cluster --- RS3 Number of bright galaxies used to determine RS type for both the C and L types --- T1 First brightest cluster galaxy Hubble type --- Sep1a Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm Sep1b Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm T2 Second brightest cluster galaxy Hubble type --- Sep2a Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm Sep2b Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm T3 Third brightest cluster galaxy Hubble type --- Sep3a Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm Sep3b Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm r12 Separation between the first and second most luminous cluster galaxies (1mm=67.14") mm r13 Separation between the first and third most luminous cluster galaxies (1mm=67.14") mm r23 Separation between the second and third most luminous cluster galaxies (1mm=67.14") mm Nb Number of apparent galaxies that are not among the three most luminous cluster galaxies --- Nt Number of apparent triple galaxies not among the three most luminous cluster galaxies --- n_Nt A 'n' indicates that a galaxy with a multiple nucleus is observed in the cluster --- FRS1a Basic RS type for the first subcluster in an F cluster number=1 Basic RS type: cD, B, L, C, F or I --- FRS1b Subsidiary property of RS type of FRS1 number=2 Appendage or subscript which indicates a subsidiary property : p=peculiar cD galaxy n=multiple nucleus cD galaxy s=satellite of a cD galaxy b=connected supergiant binary galaxy within a B-type cluster p=peculiarity associated with a supergiant binary galaxy or the B cluster itself a=arc shape of the line of galaxies defining an L-type cluster c=clumpy s=smooth I-type cluster --- FRS1c Number of bright galaxies used to determine FRS1 RS type for both the C and L types --- FRS2a Basic RS type for the second subcluster in an F cluster number=1 Basic RS type: cD, B, L, C, F or I --- FRS2b Subsidiary property of RS type of FRS2 number=2 Appendage or subscript which indicates a subsidiary property : p=peculiar cD galaxy n=multiple nucleus cD galaxy s=satellite of a cD galaxy b=connected supergiant binary galaxy within a B-type cluster p=peculiarity associated with a supergiant binary galaxy or the B cluster itself a=arc shape of the line of galaxies defining an L-type cluster c=clumpy s=smooth I-type cluster --- FRS2c Number of bright galaxies used to determine FRS2 RS type for both the C and L types --- FRS3a Basic RS type for the third subcluster in an F cluster number=1 Basic RS type: cD, B, L, C, F or I --- F3RS3b Subsidiary property of RS type of FRS3 number=2 Appendage or subscript which indicates a subsidiary property : p=peculiar cD galaxy n=multiple nucleus cD galaxy s=satellite of a cD galaxy b=connected supergiant binary galaxy within a B-type cluster p=peculiarity associated with a supergiant binary galaxy or the B cluster itself a=arc shape of the line of galaxies defining an L-type cluster c=clumpy s=smooth I-type cluster --- F3RS3c Number of bright galaxies used to determine FRS3 RS type for both the C and L types --- Other Other source data number=4 c: presence of a comment concerning the cluster in "notes" file r: continuum radio emission in a passband centered at a frequency of 1400MHz was detected in the survey by Owen et al. (1982) u: the cluster was observed but not detected at the sensitivity limit of 0.10Jy in the 1400MHz radio survey by Owen et al. (1982) v: the cluster is listed in the catalog of Leir and van den Bergh (1977) x: X-ray emission was detected in the HEAO 1 2-6 keV passband survey of Abell clusters by Johnson et al. (1983) z: the redshift of the cluster is contained in the catalog compiled by Struble and Rood (1986a) --- Abell Abell cluster identification --- u_Abell Uncertainty flag on F type of the cluster (RS1 in table1) --- m_Abell Component of the cluster number=1 M for middle --- RS Basic revised RS type --- T1 First brightest cluster galaxy Hubble type --- SepT1a Separation, see note number=2 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm SepT1b Separation, see note number=2 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm T2 Second brightest cluster galaxy Hubble type --- SepT2a Separation, see note number=2 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm SepT2b Separation, see note number=2 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm T3 Third brightest cluster galaxy Hubble type --- SepT3a Separation, see note number=2 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm SepT3b Separation, see note number=2 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively mm r12 Separation between the first and second most luminous cluster galaxies (1mm=67.14") mm r13 Separation between the first and third most luminous cluster galaxies (1mm=67.14") mm r23 Separation between the second and third most luminous cluster galaxies (1mm=67.14") mm Nb Number of apparent galaxies that are not among the three most luminous cluster galaxies --- Nt Number of apparent triple galaxies not among the three most luminous cluster galaxies --- RS1 Basic RS type for the first subcluster --- RS2 Subsidiary property of RS type number=3 Appendage or subscript which indicates a subsidiary property : p=peculiar cD galaxy n=multiple nucleus cD galaxy s=satellite of a cD galaxy b=connected supergiant binary galaxy within a B-type cluster p=peculiarity associated with a supergiant binary galaxy or the B cluster itself a=arc shape of the line of galaxies defining an L-type cluster c=clumpy s=smooth I-type cluster --- RS3 Number of bright galaxies used to determine FRS1 RS type for both the C and L types --- Sep Separation of the components (1mm=67.14") mm m_Sep Component designation --- PA Position angle of the separation vector of the components deg n_PA Component designation --- Com Comments number=4 c: presence of a comment concerning the cluster in "notes" file --- Abell Abell number --- u_Abell Uncertainty flag on the type of the cluster --- n_Abell C: confused, X: probable cluster in the foreground of an Abell cluster --- RS1 Basic RS type number=1 Basic RS type: cD, B, L, C, F or I) --- RS2 Subsidiary property of RS type number=2 Appendage or subscript which indicates a subsidiary property : p=peculiar cD galaxy n=multiple nucleus cD galaxy s=satellite of a cD galaxy b=connected supergiant binary galaxy within a B-type cluster p=peculiarity associated with a supergiant binary galaxy or the B cluster itself a=arc shape of the line of galaxies defining an L-type cluster c=clumpy s=smooth I-type cluster --- RS3 Number of bright galaxies used to determine RS type for both the C and L types --- T1 First brightest cluster galaxy Hubble type --- SepT1a Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively --- T2 Second brightest cluster galaxy Hubble type --- SepT2a Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively --- T3 Third brightest cluster galaxy Hubble type --- SepT3a Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively --- SepT3b Separation, see note number=3 The number following a 'b' or 's' designation is the measured separation (1mm=67.14") between the components of a binary galaxy or between a cD_s_ galaxy ant its nearby satellite, respectively --- r12 Separation between the first and second most luminous cluster galaxies (1mm=67.14") --- r13 Separation between the first and third most luminous cluster galaxies (1mm=67.14") --- r23 Separation between the second and third most luminous cluster galaxies (1mm=67.14") --- Nb Number of apparent galaxies that are not among the three most luminous cluster galaxies --- FRS1a Revised RS type for the first subcluster --- FRS1c Number of bright galaxies used to determine FRS1 RS type for both the C and L types --- FRS2a Revised RS type for the second subcluster --- FRS2c Number of bright galaxies used to determine FRS2 RS type for both the C and L types --- Com Comments number=4 c: presence of a comment concerning the cluster in "notes" file --- Patricia Bauer CDS 1995Jan20Struble M.F., Rood H.J. First prepared by W.H. Warren (ADC/NASA) VII_96.xml