Extended envelopes around Galactic Cepheids - V. Multi-wavelength and time-dependent analysis of IR excess

Home

All issues

Volume 651 (July 2021)

A&A, 651 (2021) A113

Full HTML

Free Access

Table D.1.

References for the photometric, spectroscopic, effective temperature and angular diameter measurements used in this study.

Star	Ref. phot.	Ref. RVs	Ref. T_eff	Ref. θ	Star	Ref. phot.	Ref. RVs	Ref. T_eff	Ref. θ
η Aql	2,3,4,5,6,7,9,10,12,14	14,20,21,37	19	43,45 ⁽ⁱ⁾	S Nor	1,2,3,7,9 ^(a,^b),10 ^(c,^d),11,12,18	29,44	19	44 ⁽ⁱ⁾
FF Aql	1,2,3,5,7,10 ^(d),12,14,18 ^(k),46,47	14,44,48	19	49,57	TW Nor	3,7,9 ^(a,^b),10 ^(c),11,12,15	29,38	19	–
FM Aql	1,2,3,4,5,6,7,8,9,10	20,21,22	19	–	V340 Nor	1,3,11,12	29,38	19	–
FN Aql	1,2,3,4,5,6,7,9,10	20,22	19	–	Y Oph	1,2,3,5,7,9,10,11,12,13,54	21,28	19	55 ⁽ⁱ⁾,56 ⁽ⁱ⁾
SZ Aql	1,2,3,4,5,6,7,8,9 ^(a,^b),10 ^(c,^d),11,12	20	19	–	RY Sco	1,2,3,5,9 ^(a,^b),10,11,13	26	19	–
TT Aql	1,2,3,4,5,6,7,8,9 ^(e),10,13,14	20,22,23	19	–	RU Sct	1,2,3,5,8,11,12	22,38	19,39	–
U Aql	2,3,5,7,8,9 ^(a,^b),10,12,14,18 ^(j)	44	19	44 ⁽ⁱ⁾	GY Sge	3,7,11,12 ^(l)	22,38	19	–
RT Aur	1,2,3,4,5,6,8,9 ^(a,^b),10 ^(c,^d),12,14,18	14,21,22	19	53 ⁽ⁱ⁾	S Sge	1,2,3,4,5,6,7,10 ^(c,^d),12,14	20,21,22	19	–
ℓ Car	2,3,9,10,11,12,15,18,58	21,24,50,51,52	19	43,51	BB Sgr	1,2,3,5,7,9 ^(a,^b),10 ^(d),16,18	22,23	19	–
U Car	1,2,3,9 ^(a,^b),10 ^(c,^d),11,12,13,15,18,36	13,21,24	19,30	44 ⁽ⁱ⁾	U Sgr	1,2,3,5,8,9 ^(a,^b),11,12,16,18 ^(k)	23,24,29	19	–
V Car	1,2,3,9 ^(a,^b),10,11	25	19	–	W Sgr	1,2,3,5,7,10,12,18 ^(k)	28,29,44	19	43,44 ⁽ⁱ⁾
VY Car	1,2,3,9 ^(a,^b),11,13,15,18	24,26	19	–	WZ Sgr	1,2,3,5,7,8,11,12,13	22,24,26	32	–
CF Cas	1,2,3,8,9 ^(h),10 ^(c),12	22,29	19	–	X Sgr	1,2,3,5,9,10,12,36,40	21	19	43,44 ⁽ⁱ⁾
DL Cas	1,2,3,5,6,8,10 ^(c),12	21,22,29	19	–	Y Sgr	1,2,3,5,7,9 ^(a,^b),10 ^(c,^d),12	21	19
V Cen	1,2,3,9 ^(a,^b),10 ^(d),11,12,16,18	24,27	19,31	–	ST Tau	1,2,3,4,5,6,8,9 ⁽ⁿ⁾,10	22,29	19	–
XX Cen	1,2,3,9,10,11,13	24 ^(f)	19	–	SZ Tau	1,2,3,4,5,6,9 ^(a,^e),10,11,14,18 ^(j)	22,29	19	–
δ Cep	2,3,4,5,6,9 ^(a,^b),10,12,18,40	41	19	42 ⁽ⁱ⁾	RY Vel	1,2,3,9,11,15	13,33	19	–
CD Cyg	1,2,3,5,6,7,8,9 ^(a,^b),10,12	26 ^(f)	19	–	RZ Vel	1,2,3,9 ^(a,^b),10,11,15	21,24,34	19	–
X Cyg	1,2,34,5,6,7,10 ^(c,^d),12,14,18 ^(k)	20,21,22,29,37	19	–	T Vel	1,2,3,9,11,35	34	19	–
β Dor	1,2,3,9 ^(a,^b),10,11,12,17,18	21,28,29	19	43	S Vul	3,8,9 ^(a,^b),10 ^(d),11,12	21,22,26	19	–
ζ Gem	2,3,5,6,9,1010 ^(d),12,14,18 ^(m),40	21,22,23,29	19		SV Vul	1,2,3,4,5,6,7,8,9 ^(a,^b),10,11,12,14,	20,22,29,37	19
CV Mon	1,2,3,5,6,8,9,10 ^(c),11,	37,38	19,39	–	T Vul	1,2,3,4,7,9 ^(a,^b),10,12,46	14,29	19	53 ⁽ⁱ⁾,57 ⁽ⁱ⁾
T Mon	1,2,3,5,9 ^(a,^b),11,12,13,18,24	23 ^(g)	32	44 ⁽ⁱ⁾	U Vul	1,2,3,4,5,6,8,9 ^(a,^b),10,14	20,21,22,29	19	–

Notes. 1- Gaia Collaboration (2018). 2- van Leeuwen et al. (1997). 3- Berdnikov (2008). 4- Barnes et al. (1997). 5- Moffett & Barnes (1984). 6- Szabados (1980). 7- Welch et al. (1984). 8- Monson & Pierce (2011). 9- Wright et al. (2010). 10- Ishihara et al. (2010). 11- Laney & Stobie (1992). 12- Monson et al. (2012). 13- Coulson & Caldwell (1985). 14- Kiss (1998). 15- Madore (1975). 16- Gieren (1981). 17- Shobbrook (1992). 18- Marengo et al. (2010a). 19- Luck (2018). 20- Barnes et al. (2005). 21- Borgniet et al. (2019). 22- Gorynya et al. (1998). 23- Storm et al. (2011). 24- Bersier (2002). 25- Lloyd Evans (1980). 26- Anderson et al. (2016a). 27- Gieren (1981). 28- Petterson et al. (2005). 29- Bersier et al. (1994). 30- Usenko et al. (2011). 31- Usenko et al. (2013). 32- Kovtyukh et al. (2005). 33- Pont et al. (1994). 34- Szabados et al. (2013). 35- Gieren (1985). 36- Gallenne et al. (2012a). 37- Storm et al. (2004). 38- Metzger et al. (1992). 39- Genovali et al. (2014). 40- Feast et al. (2008). 41- Anderson et al. (2015). 42- Mérand et al. (2005). 43- Kervella et al. (2004). 44- Gallenne et al. (2019). 45- Lane et al. (2002). 46- Szabados (1977). 47- Szabados (1991). 48- Evans et al. (1990). 49- Gallenne et al. (2012b). 50- Anderson (2014). 51- Anderson et al. (2016b). 52- Anderson (2016). 53- Gallenne et al. (2015). 54- Fernie et al. (1995). 55- Mérand et al. (2007). 56- Gallenne (2011). 57- Gallenne et al. (2012b). 58- Kervella et al. (2009).

^(a)

Band W₁ excluded due to very large error bar.

^(b)

Band W₂ excluded due to very large error bar.

^(c)

Band S₉ excluded due to very large error bar.

^(d)

Band L₁₈ excluded due to very large error bar.

^(e)

Band W₂ excluded as not consistent with other photometric values, too high value.

^(f)

Orbital motion was substracted, see text.

^(g)

We did not succeed in removing the orbital motion, so we only use recent measurements with the good phase coverage.

^(h)

Band W₄ excluded due to very large error bar.

⁽ⁱ⁾

Converted to limb-darkened diameter using the linear law approximation from Hanbury Brown et al. (1974) and the u_λ coefficient from Claret & Bloemen (2011). Stellar parameters used for choosing u_λ are (Luck 2018): v_turb = 4 m s⁻¹, [Fe/H] = 0, T_eff = 6000 K and log g = 2.0 for RT Aur, T Vul, FF Aql, δ Cep and U Aql, T_eff = 5500 K and log g = 2.0 for S Nor, T_eff = 5250 K and log g = 1.0 for T Mon and ℓ Car, T_eff = 5000 K and log g = 1.0 for U Car, T_eff = 6000 K and log g = 1.5 for Y Oph and η Aql,

^(j)

IRAC 5.8 μm, 8 μm and MIPS 70 μm were rejected as they are not consistent with other photometric values (≃0.05 mag offset).

^(k)

IRAC 5.8 μm and 8 μm were rejected as they are not consistent with other photometric values (more than −0.05 mag offset).

^(l)

Not used as not consistent with other photometric values (more than −0.05 mag offset)

^(m)

MIPS 70 μm rejected as too large errorbar

⁽ⁿ⁾

Band W₄ excluded due to very large error bar.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.