Variability long period variables (gaiadr2.vari_long_period_variable)
The table has 89617 rows, 9 columns.
Description
This table describes the Long Period Variable stars.
Some entries can be NaN when absent.
Attribution
If you have used Gaia data in your research, please use the following acknowledgement:
This work has made use of data from the European Space Agency (ESA) mission Gaia (http://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
More information can be found on the credit and citation instructions page.
Columns
| Name | Type | UCD | Unit | Description |
|---|---|---|---|---|
| solution_id | long | meta.version |
Solution Identifier |
|
| source_id | long |
meta.id meta.main meta.ref |
Unique source identifier |
|
| abs_mag_bol | double | phot.mag.bol | Magnitude[mag] |
Absolute bolometric magnitude of the star |
| abs_mag_bol_error | double |
phot.mag.bol stat.error |
Magnitude[mag] |
Error of absolute bolometric magnitude |
| rsg_flag | boolean | meta.code.status |
Red supergiant flag |
|
| bolometric_corr | double | phot.mag.bc | Magnitude[mag] |
Bolometric correction for LPVs |
| bolometric_corr_error | double |
phot.mag.bc stat.error |
Magnitude[mag] |
Error of the bolometric correction |
| frequency | double | Frequency[day^-1] |
Frequency of the LPV |
|
| frequency_error | double | Frequency[day^-1] |
Error on the frequency |