double-lined spectroscopic binary
C41461
concept
A double-lined spectroscopic binary is a binary star system in which spectral lines from both stars are visible and shift periodically due to their orbital motion around a common center of mass.
All labels observed (3)
| Label | Occurrences |
|---|---|
| spectroscopic binary star system | 2 |
| O-type star binary | 1 |
| double-lined spectroscopic binary canonical | 1 |
Description generation (CDg)
The one-sentence description above was generated by prompting gpt-5.1 with the class name and this instruction.
Instruction
generate a one-sentence description for a given conceptual class. # Response Format Return only the sentence: "Description: [one-sentence description of the conceptional class]"
Input
Class: double-lined spectroscopic binary
Generated description
A double-lined spectroscopic binary is a binary star system in which spectral lines from both stars are visible and shift periodically due to their orbital motion around a common center of mass.
Instances (3)
| Instance | Via concept surface |
|---|---|
| HD 24760 | — |
| Plaskett’s Star | spectroscopic binary star system |
|
59 Cygni as a spectroscopic binary
surface form:
59 Cygni
|
spectroscopic binary star system |