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EntityQ568196· pop 35· linked from 488 articles

galaxy

In the Vinony graph

Vinony's link graph records 488 inbound references to NGC 1407, and connects out to list of NGC objects (1001–2000), epoch and NGC 1854.

It sits within the topics Elliptical galaxies, Eridanus (constellation) and Eridanus Group.

Vinony links it to 34 Wikipedia language editions.

Key facts

Constellation
Eridanus
Right ascension
03 40 11.9
Declination
−18 ° 34 ′ 48 ″
Redshift
1,779 ± 9 km / s
Distance
76 Mly (23.3 Mpc )
Type
E0
Apparent size v
4′.6 × 4′.3

via Wikipedia infobox

Wikidata facts

Distance from Earth
18
Image
Color cutout hst 9427 02 acs wfc f814w f435w sci NGC 1407.jpg
Show 9 more facts
time of discovery or invention
1785-10-06
catalog code
GSC 05877-00735
radial velocity
1734
Commons category
NGC 1407
redshift
0.005934
apparent magnitude
6.702
galaxy morphological type
E0
right ascension
55.0496000
declination
-18.5803778

via Wikidata · CC0

~1 min read

Encyclopedic overview

NGC 1407 is an elliptical galaxy in Eridanus. It is at a distance of 76 million light-years from Earth. It is the brightest galaxy in the NGC 1407 Group, part of the Eridanus Group, with NGC 1407 being its brightest member. NGC 1400, the second-brightest of the group lies 11.8 arcmin away.

NGC 1407 is X-ray luminous, with high hot gas Fe abundance, and with evidence of recurrent radio outbursts. In the central area of the galaxy are present old stars, with mean age 12.0 ± 1.1 Gyrs, that are metal rich and with supersolar abundances of α-elements. Observations indicate that NGC 1407 hasn't recently undergone strong star-formation activity. The galaxy hosts a supermassive black hole with a mass 1.12 ± 0.42 billion solar masses, based on velocity dispersion.

Excerpted from Wikipedia’s “NGC 1407” article, available under the CC BY-SA 4.0 licence.

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