Table A.1
Seventy Algols and Algol-like Be stars with a WISE source counterpart sorted by declination.
| V* name | 2MASS | HD/BD | Spec. type | Ref. |
|
|
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| BP Mus | J12503772-7146186 | 3 | ||
| DW Aps | J17233003-6755448 | HD 156545 | B6III | 2, 3 |
| EP TrA | J15492615-6415574 | HD 140809 | A0 | 2, 3 |
| AN Tuc | J23302225-5825346 | HD 221184 | A5III | 2, 3 |
| R Ara | HD 149730 | B9IV | 1, 2, 3 | |
| UZ Nor + | J16281156-5319215 | B? | 3 | |
| V646 Cen | J11365877-5312354 | HD 100987 | B8IV | 2, 3 |
| RV Pic | J04572970-5208458 | HD 32011 | A1V | 2, 3 |
| CZ Vel *+ | J09104446-5042405 | B3 | 3 | |
| KV Pup | J07471912-4832122 | HD 63562 | A0IV | 2, 3 |
| TT Hor | J03270438-4552566 | 3 | ||
| DN Vel | J09193768-4540477 | HD 80692 | A0III | 2, 3 |
| VY Mic | J20490707-3343543 | HD 198103 | A4III | 2, 3 |
| DM Pup | J08070409-2531522 | A2.5 | 3 | |
| AA Pup | J08013612-2443034 | HD 66226 | F3IV | 2, 3 |
| YY CMa | J07005186-1914315 | A2V | 3 | |
| AO Eri | J04320093-1744475 | A2 | 2, 3 | |
| SS Lep + | J06045913-1629039 | HD 41511 | A1V | 1 |
| W Ser + | J18095070-1533009 | HD 166126 | F5III | 1, 2, 3 |
| RY Sct + | J18253147-1241241 | HD 169515 | O9.7Ibep | 1, 2, 3 |
| XY Pup | HD 67862 | A3 | 1, 2, 3 | |
| V644 Mon | J06570938-1049281 | HD 51480 | Ape | 1 |
| AW Mon | BD-10 2233 | A2 | 2, 3 | |
| RZ Sct | J18263352-0912060 | HD 169753 | B3Ib | 1, 2, 3 |
| XZ Aql | J20221335-0721034 | HD 193740 | A2 | 2, 3 |
| V696 Mon *+ | J06041349-0642321 | HD 41335 | B2Vne | 1 |
| AR Mon | J07204845-0515357 | HD 57364 | K0II | 2, 3 |
| AU Mon | J06545471-0122328 | HD 50846 | B4IV | 1, 2, 3 |
| V509 Mon + | J06471071-0102147 | G4IV | 3 | |
| π Aqr *+ | J22251662+0122389 | HD 212571 | B1Ve | 1 |
| AC Tau | J04370635+0141311 | A8 | 2, 3 | |
| SS Cet | HD 17513 | A2 | 2, 3 | |
| AX Mon | J06303293+0552012 | HD 45910 | B2III | 1 |
| DN Ori | J06002835+1013049 | HD 40632 | A2e | 1, 2, 3 |
| FM Ori | J05085439+1033341 | HD 241071 | A5 | 3 |
| V930 Oph | J18414565+1202111 | 3 | ||
| BI Del | J20273862+1420091 | G0 | 2, 3 | |
| AL Leo | J09581290+1817282 | F5 | 2, 3 | |
| U Sge | J19184840+1936377 | HD 181182 | B7.5V | 1, 2, 3 |
| AL Gem | J06573855+2053325 | HD 266913 | F6V | 2, 3 |
| RS Vul | J19174000+2226284 | HD 180939 | B5V | 2, 3 |
| DH Her + | J18473455+2250458 | HD 343047 | A5 | 2, 3 |
| RW Tau | J04035432+2807334 | HD 25487 | B8Ve | 1, 2, 3 |
| U CrB | J15181133+3138492 | HD 136175 | B6V | 1, 2, 3 |
| BC Aur | J05461654+3250500 | 3 | ||
| RX Gem | J06501154+3314207 | HD 49521 | A0 | 1, 2, 3 |
| CG Cyg | J20581343+3510298 | G9.5V | 2, 3 | |
| V367 Cyg + | J20475958+3917156 | HD 198288 | A3Ibep | 1, 2 |
| AB Per | J03374520+4045494 | HD 275604 | A5 | 2, 3 |
| SX Aur *+ | J05114292+4209553 | HD 33357 | B1Vne | 1, 2, 3 |
| RW Per | J04201676+4218517 | HD 276247 | A2 | 1, 2, 3 |
| TX UMa | J10452050+4533586 | HD 93033 | B8V | 1, 2, 3 |
| GK And | J23534719+4534458 | 3 | ||
| V995 Cyg | J19483443+4613424 | B8 | 3 | |
| SW Cyg | J20065793+4617581 | HD 191240 | A2 | 1, 2, 3 |
| IM Aur | J05152973+4624214 | HD 33853 | B9 | 2, 3 |
| RY Per | J02454210+4808379 | HD 17034 | B8V | 1, 2, 3 |
| KX And | J23070621+5011324 | HD 218393 | B3pe | 1 |
| ϕ Per *+ | J01433964+5041192 | HD 10516 | B1.5Ve | 1 |
| AY Per | J03102513+5055543 | HD 232756 | B9 | 2, 3 |
| CX Dra *+ | J18464309+5259166 | HD 174237 | B2.5Ve | 1, 3 |
| V442 Cas + | J23401479+5357339 | A0 | 3 | |
| SX Cas | J00104207+5453293 | HD 232121 | B5 | 1, 2, 3 |
| DM Per | J02255800+5606099 | HD 14871 | B5V | 2, 3 |
| GG Cas | BD+55 274 | B5 | 2, 3 | |
| RX Cas | J03074573+6734387 | A5III | 2, 3 | |
| XY Cep | J23523291+6856015 | B8 | 2, 3 | |
| SS Cam | J07162474+7319570 | G1III | 2, 3 | |
| XZ Cam | J05171266+7550053 | A0 | 2, 3 | |
| RS Cep | J05060320+8014524 | A5III | 1, 2, 3 | |
| TY UMi | J15175751+8351340 | HD 138818 | F0 | 3 |
Notes. Objects marked with an asterisk (*) show extended emission in WISE W4, while the plus sign (+) marks objects with a WISE W4/W1 flux ratio which is above the black-body law (see Table 6 in D15).
Reference. References: (1): Harmanec (2001); (2): Brancewicz & Dworak (1980); (3): Budding et al. (2004).
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