Table A.1.
Sample of bona fide stellar sources with a period analysis based on WISE data, general information (first entries).
| Ra | Dec | Identifiers | Dist | ObjType | 2M | GLP | Aka | MSX | MGL | HGL | Vb | Vr | LRS | Spec. Type | Comment |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (″) | (″) | (″) | (″) | (″) | (″) | (″) | (km s−1) | (km s−1) | |||||
| 19.463942 | 67.231448 | IRAS01144+6658 RAFGL190 | 0.22 | C | 1.1 | 1.7 | nd | nd | U | ||||||
| 124.826307 | -21.737399 | IRAS08171-2134 RAFGL5250 | 0.30 | C | 0.3 | 0.1 | - | - | U | ||||||
| 237.773837 | -56.890007 | IRAS15471-5644 | 0.20 | Can.C | 0.2 | 1.2 | 0.9 | nd | nd | U | |||||
| 287.486914 | 9.447611 | IRAS19075+0921 RAFGL2333 | 0.03 | C | 0.0 | 1.2 | 0.8 | 1.6 | - | - | U | ||||
| 323.345002 | 56.743063 | IRAS21318+5631 RAFGL5625S | 0.51 | C | 1.1 | 0.5 | nd | nd | U | C | |||||
| 349.802533 | 17.192628 | IRAS23166+1655 RAFGL3068 | 0.33 | C | 0.3 | 0.7 | - | - | C | ||||||
| 89.161446 | -67.892776 | IRAS05568-6753 | 0.23 | C | 1.9 | 3.4 | - | - | |||||||
| 82.407959 | -72.831322 | ERO0529379 IRAS05305-7251 | 0.17 | C | 0.7 | 1.4 | - | - | q(6) | ||||||
| 87.608788 | -69.934212 | ERO0550261 IRAS05509-6956 | 0.16 | C | 0.8 | 0.7 | - | - | q(6) | ||||||
| 79.701599 | -69.559563 | ERO0518484 IRAS05191-6936 | 0.30 | C | 1.5 | 3.1 | - | - | |||||||
| 87.249886 | -70.556229 | IRAS05495-7034 | 0.77 | AGB | 0.6 | - | - | ||||||||
| 75.631233 | -68.093285 | ERO0502315 SSTISAGE1CJ050231.47-680535.9 | 0.04 | AGB | 1.1 | 3.3 | - | - | |||||||
| 76.023376 | -68.394501 | ERO0504056 IRAS05042-6827 | 0.16 | C | 1.1 | - | - | ||||||||
| 81.419411 | -70.140877 | ERO0525406 IRAS05260-7010 | 0.15 | C | 0.4 | 2.3 | - | - | |||||||
| 78.257469 | -69.564110 | IRAS05133-6937 | 0.28 | C | 0.8 | - | - | ||||||||
| 79.548790 | -70.507469 | ERO0518117 IRAS05187-7033 | 0.12 | C | 0.7 | - | - | ||||||||
| 82.684006 | -71.716766 | IRAS05315-7145 | 0.32 | AGB | 0.6 | - | - | q(6) | |||||||
| 281.468597 | -1.778703 | IRAS18432-0149 OH30.7+0.4 | 1.31 | OH/IR | 1.3 | 0.8 | 1.3 | 49.5 | 84.1 | A | |||||
| 282.174774 | -2.841357 | IRAS18460-0254 OH30.1-0.7 RAFGL5535 | 0.06 | OH/IR | 1.0 | 1.0 | 1.2 | 78.5 | 118.9 | ||||||
| 282.859344 | -1.064581 | IRAS18488-0107 OH32.0-0.5 | 0.36 | OH/IR | 0.6 | 0.8 | 0.7 | 55.2 | 95.8 | A | |||||
| 283.092775 | -0.236713 | IRAS18498-0017 OH32.8-0.3 RAFGL5540 | 0.37 | OH/IR | 0.4 | 0.8 | 1.0 | 1.5 | 45.6 | 76.0 | H | ||||
| 287.284637 | 8.276116 | GPSR042.309-0.133 | 0.78 | Radio | 1.7 | 1.2 | 0.3 | 42.3 | 75.3 | ||||||
| 23.463343 | 62.448162 | IRAS01304+6211 OH127.8-0.0 RAFGL230 | 0.19 | OH/IR | 0.2 | 0.2 | 0.2 | -65.2 | -43.0 | A | |||||
| 53.377491 | 60.335957 | IRAS03293+6010 OH141.7+3.5 RAFGL5097 | 0.61 | Mira | 0.1 | 0.8 | -69.1 | -44.9 | A | ||||||
| 79.197746 | 45.567860 | IRAS05131+4530 RAFGL712 | 0.22 | OH/IR | 0.2 | nd | nd | F | |||||||
| 111.101738 | -20.198791 | IRAS07222-2005 | 0.45 | Star | 0.4 | 0.6 | 1.5 | 76.9 | 93.2 | E | M9: | ||||
| 266.099701 | -31.927624 | IRAS17411-3154 RAFGL5379 | 4.13 | OH/IR | 0.7 | 0.6 | -39.2 | -2.7 | |||||||
| 280.309784 | -6.250149 | IRAS18385-0617 OH26.2-0.6 | 0.22 | OH/IR | 0.2 | 2.0 | 1.3 | 0.9 | 49.8 | 93.0 | |||||
| 277.128905 | -9.970644 | IRAS18257-1000 OH21.5+0.5 | 0.00 | OH/IR | 1.1 | 0.7 | 1.8 | 97.6 | 134.0 | ||||||
| 51.285198 | 65.535362 | IRAS03206+6521 OH138.0+7.2 RAFGL5093 | 0.35 | OH/IR | 0.4 | 0.6 | -46.4 | -27.6 | A | ||||||
| 0.441592 | 62.748863 | IRAS23592+6228 | 2.27 | Star | 0.1 | 0.9 | 1.4 | - | - | F | |||||
| 3.853554 | 54.906147 | IRAS00127+5437 | 0.21 | Star | 0.1 | 0.2 | - | - | E | ||||||
| 4.963700 | 65.991821 | IRAS00170+6542 | 0.20 | Can.PAGB | 0.1 | 1.2 | 1.5 | -65.0 | -37.6 | E |
Notes. Column 16. References for extragalactic catalogues (‘Q’ marks probable QSOs, ‘q’ marks candidate QSOs). (1) Flesch (2015), (2) Bailer-Jones et al. (2019), (3) Guo et al. (2018), (4) Assef et al. (2018), (5) Gaia Collaboration (2021b), and (6) Solarz et al. (2017). None of the sources is listed in the QSO catalogues of Véron-Cetty & Véron (2010), Gattano et al. (2018), and Lyke et al. (2020). The full table is available at the CDS.
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