spectroscopic binary
C41599
concept
A spectroscopic binary is a binary star system whose components are too close to be visually separated but are detected and studied through periodic Doppler shifts in their spectral lines.
All labels observed (2)
| Label | Occurrences |
|---|---|
| spectroscopic binary canonical | 12 |
| binary star | 2 |
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: spectroscopic binary
Generated description
A spectroscopic binary is a binary star system whose components are too close to be visually separated but are detected and studied through periodic Doppler shifts in their spectral lines.
Instances (14)
| Instance | Via concept surface |
|---|---|
|
EQUULEUS
surface form:
Delta Equulei
|
binary star |
| ζ Persei | — |
| o Persei | — |
| HD 23180 | — |
| HD 24760 | — |
| 9 Sagittarii | — |
| Beta Centauri | — |
| Epsilon Canis Majoris | — |
| V* del Ori | — |
| HD 36486 | — |
| Algol | — |
|
variable star Algol
surface form:
Algol
|
— |
| Regulus | — |
|
59 Cygni as a spectroscopic binary
surface form:
59 Cygni
|
binary star |