J/A+AS/65/349 Markarian galaxies and Zwicky clusters relations (Petrosian+ 1986)
On the relation of Markarian galaxies with Zwicky clusters. I. Data
Petrosian A.R., Turatto M.
<Astron. Astrophys. Suppl. Ser. 65, 349 (1986)>
=1986A&AS...65..349P 1986A&AS...65..349P (SIMBAD/NED BibCode)
ADC_Keywords: Galaxies, Markarian ; Clusters, galaxy
Keywords: Markarian galaxies - clusters of galaxies.
Abstract:
In the same area covered by Markarian survey and CGCG, there are 1344
Markarian galaxies, of which 597 are positioned inside the contours of
Zwicky clusters. Data on these galaxies and respective clusters are
presented in different tables, according to whether they are galaxies
which are members of clusters, or probable or possible members
projection cases are considered separately.
File Summary:
--------------------------------------------------------------------------------
FileName Lrecl Records Explanations
--------------------------------------------------------------------------------
ReadMe 80 . This file
table1 100 180 Markarian galaxies which are real members of
the Zwicky clusters with only one redshift
value determined with more than one galaxy
(counting Markarian galaxies)
table2 82 88 Cases in which clusters have two or more values
of mean velocity in B-PPV (Baieisi-Pillastrini
et al., 1984A&AS...56..363B 1984A&AS...56..363B) and their
differences are more the 200km/s. Markarian
galaxies is a member of one subgroup
table3 111 61 Cases of Markarian galaxies which are members
of foreground or background groups containing
more than one galaxy. All these groups are
from the notes of B-PPV
table4 86 20 Cases in which Markarian galaxy is the only
object with measured redshift in the cluster
table5 73 16 Markarian galaxies which are probable members
of clusters (2000km/s<{DELTA}V<4000km/s)
table6 94 57 Markarian galaxies which are projected on the
cluster (V>4000km/s)
table7 76 248 All cases in which Markarian galaxy is
positioned within the contours given in the
Zwicky catalogue, but there are no velocities
either for the cluster or for the galaxy or
for either of them
ref 71 19 Reference for velocities
--------------------------------------------------------------------------------
See also:
VII/172: First Byurakan Survey (FBS) (Markarian+, 1989)
I/49 : Galaxies and Clusters of Galaxies (CGCG) (Zwicky, 1968)
Byte-by-byte Description of file: table1
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Cluster Cluster designation by right ascension and
declination (1950)
12- 15 A4 --- n_Cluster Note on Cluster
17- 24 A8 --- Type Cluster type
25- 29 I5 km/s HRVc Cluster heliocentric radial velocity
30 A1 --- n_HRVc ['] Note on HRVc (1)
32- 37 A6 --- NGal Number of galaxies with published redshifts
used to compute the mean HRV
39- 43 I5 --- Mrk Markarian galaxy designation (see Cat. VII/172)
45- 49 I5 km/s HRVm Markarian galaxy heliocentric radial velocity
51- 52 I2 --- r_HRVm [1/14] References of the Markarian galaxy
velocity (See ref file)
53 A1 --- Note [*] * : individual note (2)
55-100 A46 --- Notes Notes (3)
--------------------------------------------------------------------------------
Note (1): ': Cluster velocities recalculated with velocities of Markarian
galaxies which are new members of clusters
Note (2): Zw 0310.0-0130: Two background objects with V=9200km/s from B-PPV
were used for calculation of cluster mean velocity.
Zw 0801.3+3954: Background object with V=10020km/s from B-PPV was used
for calculation of cluster mean velocity.
Zw 0819.6+2209: Markarian galaxies are members of and
subgroups of Bothun et al. (1983ApJ...268...47B 1983ApJ...268...47B) respectively.
Zw 0837.0+2506: The galaxy with V=5420km/s is B-PPV is NGC 2623. Its
diameter is about three times that of real members of the cluster
It is probably a foreground object.
Zw 1051.4+4041: Cluster velocity taken similar to Shahbazian 1
(Kirshner and Malumuth, 1980ApJ...236..366K 1980ApJ...236..366K).
Zw 1144.0+5555: Mrk 1455 is also a member of the background group of
Zw 1138.7+5650.
Note (3): Geller-Huchra groups (GH) of galaxies, (Geller & Huchra, 1983,
Cat. VII/84), Abell clusters, Abell (1958, Cat. VII/4),
coincident with Zwicky clusters or other clusters denominations
are given
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table2
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Cluster Cluster and subgroup designation by right
ascension and declination (1950)
12 A1 --- m_Cluster Multiplicity index on Cluster
14- 20 A7 --- Type Cluster type
22- 26 I5 km/s HRVc Heliocentric radial velocity from B-PPV of
each subgroup in the cluster.
27 A1 --- n_HRVc ['] Note on HRVc (1)
29- 31 A3 --- NGal Number of galaxies with published redshifts
used to compute the mean HRV
33- 36 I4 --- Mrk ? Markarian galaxy designation (see Cat. VII/172)
38- 42 I5 km/s HRVm ? Markarian galaxy heliocentric radial velocity
44- 45 I2 --- r_HRVm ? [1/14] References of the Markarian galaxy
velocity (See ref file)
46 A1 --- Note [*] *: individual notes (2)
48- 82 A35 --- Notes Notes (3)
--------------------------------------------------------------------------------
Note (1): ': Subgroup velocities recalculated with velocities of Markarian
galaxies which are new members of the subgroup
Note (2): Zw 0826.2+3039: The diameter of Mrk 390 is 0.40mm and the mean
diameter for cluster galaxies is 0.37±0.13mm.
Zw 0926.5+3026: Mrk 401 with five other neighbours have diameters
of 1.00mm and the mean diameter for other cluster members is
0.36±0.11mm.
Zw 0957.9+1111: There are two systems of diameters, d1=0.44±0.12mm
and d2=1.00±0.10mm, in the cluster. subgroup velocity with
IC 584 (d=1.00mm); subgroup introduced by us with velocity
from Mrk 1241 (d=0.30mm).
Zw 1655.8+6844: Mrk 1110 is probably a member of V 107
({DELTA}V=2200km/s).
Zw 1707.6+4045: The diameter of Mrk 501 is 0.80mm and the mean
diameter for cluster galaxies is 0.65±0.13mm. The galaxy with
V=2110km/s is NGC 6339 (d=2.55mm). It is probably a foreground
object.
Note (3): GH (Geller & Huchra, 1983, Cat. VII/84) and V (Vennik, 1984, A List
of Nearby Groups of Galaxies, Tallin, USSR) groups, Abell clusters,
Abell (1958, Cat. VII/4), coincident with subgroups of Zwicky
clusters are given
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table3
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Cluster Designation by right ascension and
declination (1950) of cluster and subgroups
having foreground or background groups
12 A1 --- m_Cluster Multiplicity index on Cluster
14- 18 I5 km/s HRVc Heliocentric radial velocity of the cluster
or the the subgroups
19 A1 --- n_HRVc ['] Note on HRVc (1)
21- 24 A4 --- NGal Number of galaxies used to compute the
mean HRV
26- 30 I5 km/s HRVg ? Group heliocentric radial velocity
31 A1 --- n_HRVg ['] Note on HRVg (2)
33- 35 A3 --- NGal2 Number of galaxies with published redshifts
used to compute the mean HRV
37- 40 I4 --- Mrk ? Markarian galaxy designation (see Cat. VII/172)
42- 46 I5 km/s HRVm ? Markarian galaxy heliocentric radial velocity
48 I1 --- r_HRVm ? [1/14] References of the Markarian galaxy
velocity (See ref file)
49 A1 --- Note [*] * : individual notes (3)
51-111 A61 --- Notes Notes (4)
--------------------------------------------------------------------------------
Note (1): ': Subgroup velocities recalculated with velocities of Markarian
galaxies which are new members of clusters
Other velocities are from B-PPV
Note (2): ': Group velocities recalculated with velocities of Markarian
galaxies which are members of this group
Note (3): Zw 1138.7+5650: Galaxies Mrk 184, 1456 and 1457 have velocities
similar to the cluster Zw 1144.0+5555 but they are located out of
its contour. Mrk 1455 is a member of both clusters.
Zw 1424.0+2613: Mrk 673 is a member of the cluster Zw 1424+2613B
(Noonane, 1981ApJS...45..613N 1981ApJS...45..613N).
Zw 1600.4+1925: See Chincarini and Martins (1975ApJ...196..335C 1975ApJ...196..335C).
Note (4): GH (Geller & Huchra, 1983, Cat. VII/84) and V (Vennik, 1984, A List
of Nearby Groups of Galaxies, Tallin, USSR) groups coincident with
foreground or background groups.
Other cluster denominations are given
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table4
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
-------------------------------------------------------------------------------
1- 11 A11 --- Cluster Cluster designation by right ascension and
declination (1950)
13- 16 A4 --- Dist Cluster distance class
18- 24 A7 --- Type Cluster type
26- 29 I4 --- Mrk Markarian galaxy designation (see Cat. VII/172)
31- 35 I5 km/s HRVm Markarian galaxy heliocentric radial velocity
37 I1 --- r_HRVm [1/14] References of the Markarian galaxy
velocity (See ref file)
39- 42 F4.2 mm Diam Markarian galaxy diameter
44- 47 F4.2 mm Diam10 Mean value of diameters of 10 near galaxies
49- 52 F4.2 mm e_Diam10 rms uncertainty on Diam10
54 A1 --- Note [*] * : individual notes (1)
56- 86 A31 --- Notes Notes
--------------------------------------------------------------------------------
Note (1): Zw 0921.6+2354: Projection is possible (see B-PPV and Turatto and
Petrosian, 1985ATsir1371....1T 1985ATsir1371....1T).
Zw 1224.6+3131: The galaxy with V=725km/s in B-PPV is NGC 4414
(d∼4.0mm and mp=10.9). It is probably a foreground object.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table5
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Cluster Cluster designation by right ascension and
declination (1950)
12 A1 --- m_Cluster Multiplicity index on Cluster
14- 20 A7 --- Type Cluster type
22- 26 I5 km/s HRVc Cluster heliocentric radial velocity
27 A1 --- n_HRVc ['] Note on HRVc (1)
29- 33 A5 --- NGal Number of galaxies with published redshifts
used to compute the mean HRV
35- 38 I4 --- Mrk ? Markarian galaxy designation (see Cat. VII/172)
40- 44 I5 km/s HRVm ? Markarian galaxy heliocentric radial velocity
46 I1 --- r_HRVm ? [1/14] References of the Markarian galaxy
velocity (See ref file)
48- 73 A26 --- Notes Notes
--------------------------------------------------------------------------------
Note (1): ': Cluster velocities recalculated with velocities of Markarian
galaxies which are new members of clusters
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table6
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Cluster Cluster designation by right ascension and
declination (1950) (See Zwicky CGCG I/49)
12 A1 --- m_Cluster Multiplicity index on Cluster
14- 17 A4 --- Dist Cluster distance class
19- 23 I5 km/s HRVc ? Cluster heliocentric radial velocity
24 A1 --- n_HRVc ['] Note on HRVc (1)
26- 31 A6 --- NGal Number of galaxies with published redshifts
used to compute the mean HRV
33 A1 --- r_HRVc ? [A/E] References of the velocity of the cluster
(See ref file)
35- 38 I4 --- Mrk ? Markarian galaxy designation (see Cat. VII/172)
40- 44 I5 km/s HRVm ? Markarian galaxy heliocentric radial velocity
45 A1 --- n_HRVm [s] s for star
46- 50 F5.3 --- z ? Redshift instead of radial velocity
52- 53 I2 --- r_HRVm ? [1/14] References of the Markarian galaxy
velocity (See ref file)
54 A1 --- Note [*] *: individual notes (2)
56- 94 A39 --- Notes Notes
-------------------------------------------------------------------------------
Note (1): ': Cluster velocities recalculated with velocities of Markarian
galaxies which are new members of clusters
Note (2): Zw 0927.2+3446: The diameter of Mrk 399 is 0.30mm while the mean
diameter for cluster galaxies is 0.60±0.12mm.
Zw 1429.9+5256: The criterion of diameters was used. Mrk 816 may be a
member of "distant" clusters Zw 1433.4+5335 or Zw 1435.0+5203.
Zw 1552.5+3435: The velocity for the cluster in B-PPV was obtained
with Mrk 493. Its a diameters is 1.05mm, while the mean diameter
for cluster members is 0.34±0.10mm.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: table7
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 11 A11 --- Cluster Cluster designation by right ascension and
declination (1950)
12 A1 --- m_Cluster Multiplicity index on Cluster
14- 17 A4 --- Dist Cluster distance class
19- 23 I5 km/s HRVc ? Cluster heliocentric radial velocity
24 A1 --- n_HRVc ['] Note on HRVc (1)
26 A1 --- r_HRVc ? [A/E] References of the velocity of the cluster
(See ref file)
28- 31 I4 --- Mrk ? Markarian galaxy designation (see Cat. VII/172)
32 A1 --- u_Mrk Uncertainty flag on Mrk
34- 38 I5 km/s HRVm ? Markarian galaxy heliocentric radial velocity
40- 41 I2 --- r_HRVm ? [1/14] References of the Markarian galaxy
velocity (See ref file)
42 A1 --- Note [*] *: individual notes (2)
44- 76 A33 --- Notes Notes
--------------------------------------------------------------------------------
Note (1): ': Cluster velocities recalculated with velocities of Markarian
galaxies which are new members of clusters
Note (2): Zw 1043.9+5635: Mrk 35 (d=1.00mm) is a member of the group with
V=1100km/s (B-PPV) and d=1.00mm, while the mean diameter for
cluster galaxies is 0.38±0.16mm.
--------------------------------------------------------------------------------
Byte-by-byte Description of file: ref
--------------------------------------------------------------------------------
Bytes Format Units Label Explanations
--------------------------------------------------------------------------------
1- 2 A2 --- No Reference number or letter
5- 27 A23 ---- Name Author names
29- 47 A19 --- Bib Bibcode
49- 57 A9 --- Cat Catalogue number
--------------------------------------------------------------------------------
History: Prepared via OCR at CDS.
References:
Petrosian & Turatto, Paper II. Discussion =1986A&A...163...26P 1986A&A...163...26P
(End) Marie-Jose Wagner, Patricia Bauer [CDS] 14-Apr-1997