(Q88283122)

English

CNOC MS 0451 100520

galaxy

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Statements

1 reference

CNOC MS 0451 100520

1 reference

[MET2007] 73.592110-3.047124

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

1 reference

[SJV2010] J045422.088-030249.245

Cosmic chronometers: constraining the equation of state of dark energy. II. A spectroscopic catalog of red galaxies in galaxy clusters

1 reference

0 references

0.54476

1 reference

The CNOC Cluster Redshift Survey Catalogs. VI. MS 0015.9+1609 and MS 0451.5−0305

0.5444

1 reference

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

0.5438

1 reference

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

0.544

2 references

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

Cosmic chronometers: constraining the equation of state of dark energy. II. A spectroscopic catalog of red galaxies in galaxy clusters

radial velocity

122,607 kilometre per second

1 reference

Cosmic chronometers: constraining the equation of state of dark energy. II. A spectroscopic catalog of red galaxies in galaxy clusters

galaxy morphological type

E

1 reference

apparent magnitude

20.3

astronomical filter

1 reference

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

1 reference

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

right ascension

73.5921083 degree

1 reference

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

−3.0471250 degree

1 reference

A Wide‐Field Survey of Twoz∼ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

Identifiers

CNOC MS 0451 100520

0 references

Sitelinks

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arzwiki CNOC MS 0451 100520 (مجره)

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