NGC 7619 is an elliptical galaxy located in the constellation Pegasus.[2] NGC 7619 and NGC 7626[3] are the dominant and brightest members of the Pegasus galaxy cluster.[4] Both of them were discovered by William Herschel on September 26, 1785.[5]
The radial velocity of this galaxy was measured in 1929 and found to be double that of any galaxy observed at that time.[6] The measurement was consistent with the extrapolated value predicted by Edwin Hubble; a distance-velocity relation that would later become known as Hubble's Law.[7]
In 1970, a type Ia supernova was detected within NGC 7619; it was subsequently designated SN 1970J.[8]
^ abcdefg"NGC 7619". Simbad. Université de Strasbourg/CNRS. Retrieved 2021-02-10.
^Cite error: The named reference Hodge was invoked but never defined (see the help page).
^Cite error: The named reference Randall was invoked but never defined (see the help page).
^Cite error: The named reference Zwicky was invoked but never defined (see the help page).
^Seligman, Courtney. "New General Catalogue objects: NGC 7600 - 7649". cseligman.com. Retrieved 2021-02-10.
^Cite error: The named reference Humason was invoked but never defined (see the help page).
^Cite error: The named reference Hubble was invoked but never defined (see the help page).
^"SN 1970J". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-10.
NGC7619 is an elliptical galaxy located in the constellation Pegasus. NGC7619 and NGC 7626 are the dominant and brightest members of the Pegasus galaxy...
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