Non-conservative evolution in Algols: where is the matter?

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Volume 577 (May 2015)

A&A, 577 (2015) A55

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Table 6

2MASS and WISE magnitudes for the 13 systems deviating the most from the F_W4/F_W1 black-body law (see Fig. 13).

Name	P _orb	(Sp.1)	J	H	K _s	W1	W2	W3	W4
	(d)		(mag)	(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
	q	[Sp.2]	ϖ (mas)			[SNR_W1 ]()	[SNR_W2]()	[SNR_W3]()	[SNR_W4]()

CZ Vel	5.1927⁽¹⁾	(B3)⁽³⁾	9.441	9.192	9.032	8.562	8.485	7.814	3.669
	0.50⁽³⁾	[B6]	Unk.			[50](1.75)	[52.6](1.79)	[48.2](5.46)	[42.9](35.4)
UZ Nor	3.1960⁽²⁾	(A1)⁽²⁾	10.262	10.079	9.982	9.873	9.817	8.202	5.937
	0.18⁽³⁾	[K0IV]	Unk.			[48.3](3.27)	[57.4](2.82)	[40.8](5.7)	[22.9](1.33)
V509 Mon	4.9174⁽³⁾	(B7)⁽³⁾	12.595	12.171	11.987	11.868	11.905	11.515	8.38
	0.32⁽³⁾	[G4IV]	Unk.			[46.3](1.23)	[43.9](1.37)	[6.5](1.14)	[4.7](0.992)
DM Pup	3.567⁽¹²⁾	(B5)⁽³⁾	12.761	12.569	12.488	12.057	12.035	11.215	8.868
	Unk.	[A2.5]	Unk.			[46.1](1.38)	[42.6](1.61)	[9.6](1.00)	[3.2](1.09)
V442 Cas	3.5922⁽³⁾	(A7)⁽³⁾	11.729	11.516	11.407	11.286	11.271	10.961	8.76
	0.18⁽³⁾	[K2IV]	Unk.			[49.6](1.36)	[52.2](1.42)	[14.9](0.995)	[4.2](0.994)
DH Her	Unk.	(A5)⁽⁶⁾	10.054	9.997	9.956	10.134	10.168	10.189	8.449
	Unk.	[Unk.]	Unk.			[47.9](5.90)	[53.6](6.06)	[26.9](1.12)	[5.4](0.979)
RY Sct	11.12⁽⁸⁾	(O9.7Ibpe)⁽⁹⁾	6.245	5.854	5.463	4.955	3.895	0.014	–0.922
	0.23⁽¹⁰⁾	[O6.5 I]	1.59			[14.2](12.1)	[19.4](51.0)	[21.3](0.550)	[83.96](2.21)
V367 Cyg	18.6⁽¹³⁾	(A7I)⁽³⁾	5.202	5.006	4.828	4.72	4.038	3.781	2.676
	0.825⁽¹³⁾	[Unk.]	1.74			[13.2](0.434)	[20.9](2.34)	[70.9](1.27)	[31.4](1.24)
W Ser	14.154⁽³⁾	(B emb.)⁽¹¹⁾	7.416	6.109	5.558	5.106	4.560	4.038	3.379
	0.64⁽³⁾	[F5III]	0.70			[13.6](0.737)	[18.2](3.65)	[69](1.72)	[31.3](1.36)
SS Lep	260.3⁽⁵⁾	(A1V)⁽⁵⁾	2.094	2.105	1.671	3.455	1.536	–1.307	–2.117
	0.47⁽⁵⁾	[M6II]	3.59			[39](186)	[64.3](195)	[3](0.0094)	[962](45.2)
HR 2142	~80⁽¹⁶⁾	(B2IVne)⁽¹⁶⁾	5.088	5.068	4.781	4.828	3.756	3.31	2.592
	Unk.	[Unk.]	2.48			[12.1](15.4)	[16](25.5)	[91.1](7.12)	[58.9](1.96)
π Aqr	84.1⁽¹⁵⁾	(B1Ve)⁽⁴⁾	5.305	5.365	5.351	4.573	3.767	4.056	3.58
	0.16⁽¹⁵⁾	[A-F]⁽¹⁵⁾	4.17			[13.8](1.22)	[16](2.10)	[73.8](1.68)	[41.7](1.02)
CX Dra	6.696⁽¹⁷⁾	(B2.5Ve)⁽¹⁷⁾	5.870	5.805	5.486	5.457	5.140	5.128	4.854
	0.23⁽¹⁵⁾	[F5III]⁽¹⁷⁾	2.52			[17.4](1.27)	[32.9](2.07)	[77.9](4.48)	[49](1.11)
φ Per	127⁽¹⁴⁾	(B2e)⁽¹⁴⁾	4.049	3.955	3.709	3.68	2.774	2.639	1.869
	0.158⁽³⁾	[sdO]	4.54			[8.7](0.247)	[12.2](1.59)	[53.5](2.03)	[65.4](0.737)
SX Aur	1.21⁽⁴⁾	(B2)⁽⁴⁾	8.431	8.471	8.541	8.594	8.655	8.636	7.047
	0.61⁽⁷⁾	[B5]	1.39			[47.9](2.97)	[55.6](3.53)	[42](1.29)	[13.6](1.34)

Notes. “Unk.” refers to unknown values, “emb.” to an embedded star where the spectral type is only roughly guessed. q is the mass ratio defined as q = M_donor/M_gainer.

Reference. ⁽¹⁾Zasche (2009); ⁽²⁾Zasche (2011); ⁽³⁾Budding et al. (2004) and references therein; ⁽⁴⁾Linnell et al. (1988); ⁽⁵⁾Blind et al. (2011); ⁽⁶⁾Kreiner (2004); ⁽⁷⁾Linnell et al. (1988); ⁽⁸⁾Kreiner (2004); ⁽⁹⁾Walborn (1982); ⁽¹⁰⁾Grundstrom et al. (2007); ⁽¹¹⁾Plavec (1989); ⁽¹²⁾Hegedus (1988); ⁽¹³⁾Zoła & Ogłoza (2001); ⁽¹⁴⁾Hummel & Štefl (2001); ⁽¹⁵⁾Bjorkman et al. (2002); ⁽¹⁶⁾Waters et al. (1991); ⁽¹⁷⁾Berdyugin & Piirola (2002).

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