The structure of disks around Herbig Ae/Be stars as traced by CO ro-vibrational emission

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Volume 574 (February 2015)

A&A, 574 (2015) A75

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Table 1

Astrophysical parameters of the programme stars.

ID	Name	Sp. type	Group	log T_eff	log L_bol	M	d	i ^⋆	PA
				log [K]	log [L_⊙]	[M_⊙]	[pc]	[°]	[°]


1	HD 100546	B9Vne	I	4.02	1.62	2.4 ±0.1^o	103^y	42 ±5^d	145 ±5^d
2	HD 97048	A0pshe	I	4.00	1.42	2.5 ±0.2^o	180^y	42.8^a	175 ±1^♣
3	HD 179218	B9e	I	4.02	1.88	2.7 ±0.2ⁱ	240^y	57 ±2^u	23 ±3^u
4	HD 101412	B9.5V	II	4.02	1.40	2.3 ±0.2ⁱ	160^g	80 ±7^u	38 ±5^u
5	HD 141569^†	B9.5e		3.98	1.10	2.00^s	99^y	51 ±3^t	356 ±5^t
6	HD 190073	A2IVpe	II	3.95	1.92	2.85^l	≥290^y	23^m	10^m
7	HD 98922	B9Ve	II	4.02	2.95^‡	2.2 ±0.8^x	≥540^‡ y	45^x	–
8	HD 95881	A2III/IV	II	3.95	1.34ⁿ	2.0 ±0.3ⁿ	170 ±30ⁿ	55ⁿ	103ⁿ
9	R CrA	A5IIev	II	3.86	–	3.5^r	130^b	65^q	180^q
10	HD 135344B^†	F8V		3.82	1.01	1.7 ±0.2ⁱ	140 ±2^f	14 ±3^e	56 ±2^e
11	HD 150193	A1Ve	II	3.95	1.19	2.3 ±0.2^o	150^y	38 ±9^v	358 ±6^v
12	HD 104237	A4Ve+sh^o	II	3.92	1.53	1.96^k	116^y	18^k	–
13	HD 142666	A8Ve	II	3.88	1.03	1.8 ±0.3^o	145 ±2^f	almost edge-on^h	–

Notes. The references for the values for the effective temperature of the central star log T_eff, the observed bolometric luminosity log L_bol, and the distance d can be found in Acke et al. (2005) and references therein, unless indicated otherwise.

^(⋆)

Inclination in degrees from face-on.

^(♣)

Derived from the PAH 8.6 μm image of Lagage et al. (2006).

^(†)

We do not classify this source in group I/II (Sect. 2).

^(‡)

Ambiguity about the distance exists (Blondel & Tjin A Djie 2006).

Reference.

^(a)

Lagage et al. (2006);

^(b)

Marraco & Rydgren (1981);

^(c)

Acke & van den Ancker (2006);

^(d)

Ardila et al. (2007);

^(e)

Pontoppidan et al. (2008);

^(f)

de Zeeuw et al. (1999);

^(g)

Acke & van den Ancker (2004);

^(h)

Meeus et al. (1998);

⁽ⁱ⁾

van der Plas et al. (2008);

^(k)

Grady et al. (2004);

^(l)

Catala et al. (2007);

^(m)

Eisner et al. (2004);

⁽ⁿ⁾

Verhoeff et al. (2010);

^(o)

van Boekel et al. (2005);

^(q)

Kraus et al. (2009);

^(r)

Forbrich et al. (2006);

^(s)

Merín et al. (2004);

^(t)

Weinberger et al. (1999);

^(u)

Fedele et al. (2008);

^(v)

Fukagawa et al. (2003);

^(w)

Kraus et al. (2008);

^(x)

Blondel & Tjin A Djie (2006);

^(y)

van den Ancker et al. (1998).

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