Web Resource
URL: https://osdr.nasa.gov/bio/repo/data/studies/OSD-738
From the dataset abstract
M dwarfs are the most numerous stars in the galaxy. They are characterized by strong magnetic activity. The ensuing high-energy emission is crucial for the evolution of their planets and...
Source: UV/X-Ray Data for M Dwarfs Within 10 Parsecs
About this Resource
| Last updated | unknown |
|---|---|
| Created | unknown |
| Format | Web Resource |
| License | other-license-specified |
| Created | 2 months ago |
| Media type | application/octet-stream |
| has views | False |
| id | 0c301c07-924b-4690-a6f4-e6e686c3fb5a |
| metadata modified | 2 months ago |
| package id | 8835c986-9c26-4265-aba2-f9f34bb86522 |
| position | 2 |
| state | active |
| tracking summary | {'total': 0, 'recent': 0} |