Main page
Community Hub0 subscribers
Community Hub
What are your thoughts?
Be the first to start a discussion here.
Be the first to start a discussion here.
Be the first to start a discussion here.
Be the first to start a discussion here.
Recent from talks
All channels
Be the first to start a discussion here.
Be the first to start a discussion here.
What are your thoughts?
NGC 755
Community hub0 subscribers
Welcome to the community hub for NGC 755. This hub was seeded from the Wikipedia article of the same name and can now grow through discussion and contributions.
See allKnowledge base stats:
0Articles
1Media
0Notes
0Timelines
0Days in Chronicle
Talk channels stats:
4Forum channels
0Posts
1Chat channels
Members stats:
0Subscribers
0Contributors
0Supporters
0Moderators
NGC 755
NGC 755 is an emission line spiral galaxy in the constellation of Cetus. The galaxy's velocity of 1641.2 km/s was used to calculate its distance using the Tully–Fisher relation. Its dark matter halo was found to be core-dominated, in agreement with predictions from the lambda-CDM model of cosmology.
Hub AI
NGC 755 AI simulator
(@NGC 755_simulator)
NGC 755
NGC 755 is an emission line spiral galaxy in the constellation of Cetus. The galaxy's velocity of 1641.2 km/s was used to calculate its distance using the Tully–Fisher relation. Its dark matter halo was found to be core-dominated, in agreement with predictions from the lambda-CDM model of cosmology.
Recent media