Table 2. Open in new tab The...

Table 2.

The Sarajedini’s ID of outliers we detected in 47 Tuc that were listed in previous publications. All sources are most likely cluster members according to Bellini et al. (2014).

ID	ID_Saraj.	Previous Classifications	ID_BH17
25	57083	SPV?¹, AB², Binary⁴, CV?⁵	75
26	46102	W UMa¹	–
27	57456	Variable¹, CV?², CV (WD–MS)⁴, CV⁵	30
28	54823	CV?², Intriguing object⁴	21
29	22861	CV?², CV⁵	56
30	50798	CV?², CV?³	71

ID	ID_Saraj.	Previous Classifications	ID_BH17
25	57083	SPV?¹, AB², Binary⁴, CV?⁵	75
26	46102	W UMa¹	–
27	57456	Variable¹, CV?², CV (WD–MS)⁴, CV⁵	30
28	54823	CV?², Intriguing object⁴	21
29	22861	CV?², CV⁵	56
30	50798	CV?², CV?³	71

Note:

¹ Albrow et al. (2001), ²Edmonds et al. (2003), ³Heinke et al. (2005), ⁴Knigge et al. (2008), ⁵Sandoval et al. (2018). AB = active binaries; BY-Dra = BY Draconis variables; CV = Cataclysmic variable; CV? = Cataclysmic variable candidate; SPV = Short Period Variable; SG = Sub Giant; V = Variable; W UMa = W Ursae Majoris variable; WD–MS = White dwarf–Main-sequence binary. X-ray ID by Bhattacharya et al. 2017 (BH17).

This Feature Is Available To Subscribers Only