Table 1
Excerpt from the list of our sample of 379 Galactic classical Cepheids.
Name | αICRS | δICRS | Period [days] | Mode | [Fe/H]lit ± σ | Ref. | X [pc] | Y [pc] | Z [pc] | RH [pc] | RG [pc] | σ(R) [pc] |
---|---|---|---|---|---|---|---|---|---|---|---|---|
AAGem | 06:06:34.946 | +26:19:45.191 | 11.3128451 | 0 | −0.08 ± 0.05 | 1 | −11353 | −259 | 182 | 3245 | 11356 | 184 |
AA Ser | 18:41:21.761 | −01:06:40.442 | 17.1424446 | 0 | 0.38 ± 0.20 | 1 | −5015 | 1851 | 122 | 3618 | 5346 | 419 |
… | … | … | … | … | … | … | … | … | … | … | … | … |
1 Car | 09:45:14.782 | −62:30:28.323 | 35.5580599 | 0 | 0.24 ± 0.10 | 1 | −8013 | −465 | −38 | 481 | 8027 | 12 |
ζ Gem | 07:04:06.522 | +20:34:13.059 | 10.1485988 | 0 | 0.01 ± 0.06 | 2 | −8484 | −102 | 101 | 385 | 8485 | 4 |
Notes. The first five columns give the star name, the right ascension and declination, the pulsation period, and the pulsation mode (0: fundamental; 1: first overtone; 2: multimode; −1: no mode identification available). Columns (6) and (7) give the iron abundance from the literature and the corresponding references. The last six columns list the heliocentric X, Y, Z projected distances and the heliocentric and galactocentric radial distances together with their errors. For V1359 Aql, we have no information about the pulsation period and the error on the radial distance. The complete table is available at the CDS.
References. 1: Genovali et al. (2014): for some of the stars, we assumed a typical error of 0.1 dex because they were not provided by the original authors; 2: da Silva et al. (2022): the adopted uncertainty is the highest value between σ and std.
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