A near-infrared interferometric survey of debris-disk stars - VII. The hot-to-warm dust connection

Home

All issues

Volume 651 (July 2021)

A&A, 651 (2021) A45

Full HTML

Free Access

Table B.1

Main properties of the 62 newly observed stars.

Star	Type	Dist.	V	H	θ_LD	Age	References
		(pc)	(mag)	(mag)	(mas)	(Gyr)
HD 203	F2IV	39.0	6.181^0.003	5.32^0.05	0.347^0.005	0.021	1, 2, 3, 31, 32
HD 2834	A0V	53.0	4.751^0.008	4.76^0.07	0.381^0.006	0.22	1, 2, 3, 4
HD 3126	F5V	41.0	6.907^0.009	5.85^0.05	0.284^0.004	1.59	1, 2, 3, 4
HD 4113	G5V	44.0	7.889^0.009	6.34^0.02	0.240^0.003	5.8	5, 7
HD 4247	F0V	27.0	5.218^0.003	4.46^0.01	0.513^0.006	1.7	6
HD 9672	A1V	59.0	5.611^0.004	5.53^0.02	0.273^0.004	0.1	1, 3, 4, 8
HD 10008	K0/1V	24.0	7.66^0.01	5.90^0.04	0.324^0.005	4.2	1, 3, 9
HD 10269	F5V	48.0	7.078^0.004	5.90^0.04	0.252^0.003	1.6	1, 4
HD 10939	A1V	62.0	5.033^0.003	5.03^0.02	0.339^0.006	0.2	1, 2, 3
HD 15427	A2/3V	47.0	5.124^0.002	5.03^0.02	0.349^0.005	0.24	1, 2
HD 17848	A2V	50.5	5.252^0.004	5.16^0.08	0.350^0.005	0.28	1, 2, 3, 4, 8
HD 23484	K1V	16.0	6.982^0.004	5.09^0.02	0.484^0.006	6.9	2, 3, 8, 10, 11
HD 24649	F6V	41.0	7.217^0.007	6.09^0.03	0.261^0.004	4.8	1, 6
HD 28287	K0V	38.0	8.77^0.01	6.87^0.04	0.210^0.003	0.1	1, 3, 7
HD 29137	G5V	52.0	7.663^0.008	6.16^0.03	0.258^0.004	6.29	1, 12
HD 31203	F0IV	37.1	5.606^0.004	4.88^0.02	0.414^0.006	0.70	4, 13
HD 31392	G9V	26.0	7.600^0.008	5.89^0.04	0.317^0.005	3.70	3, 8
HD 36187	A0V	87.8	5.557^0.003	5.51^0.02	0.264^0.004	0.25	4, 14
HD 37306	A2V	63.0	6.087^0.004	5.992^0.02	0.215^0.003	0.16	1, 2, 3, 4, 8
HD 37484	F3V	57.0	7.249^0.008	6.29^0.02	0.217^0.003	0.7	1, 2, 3, 6, 8
HD 38949	G1V	43.3	7.808^0.008	6.48^0.04	0.215^0.003	0.9	2, 3, 8
HD 41278	F5V	56.0	7.394^0.008	6.36^0.03	0.220^0.003	2.3	1, 6
HD 43879	F5V	64.1	7.494^0.008	6.46^0.04	0.216^0.003	2.0	4, 15
HD 44524	F3V	102.3	7.012^0.01	6.46^0.03	0.193^0.003	1.6	6, 14, 15
HD 59967	G3V	21.8	6.657^0.004	5.25^0.02	0.412^0.006	0.63	1, 2, 3, 16, 17
HD 60491	K2V	25.0	8.15^0.01	6.14^0.02	0.298^0.005	0.08	1, 3, 18
HD 61005	G3/5V	35.3	8.215^0.008	6.58^0.04	0.228^0.004	0.1	1, 2, 3, 19
HD 71722	A0V	71.7	6.05^0.004	5.91^0.02	0.225^0.003	0.4	1, 2, 3, 4, 8, 20
HD 76143	F5IV	52.0	5.328^0.003	4.42^0.02	0.536^0.009	2.2	1, 3, 4
HD 80133	K1/2V	68.5	7.76^0.01	5.90^0.03	0.337^0.005	0.4	7, 11
HD 80883	K0V	36.2	8.59^0.01	6.63^0.05	0.242^0.004	6.3	7, 21
HD 89886	F7V	167.0	7.44^0.01	6.09^0.05	0.273^0.004	1.6	6, 7
HD 90781	F3V	77.0	7.448^0.008	6.51^0.03	0.198^0.003	1.2	4, 14, 15
HD 90874	A2V	68.0	5.991^0.004	5.86^0.04	0.237^0.003	0.25	1, 2, 3, 4, 8
HD 92945	K1V	21.4	7.708^0.007	5.77^0.05	0.347^0.005	0.21	7, 8
HD 93453	A4IV	72.0	6.288^0.004	5.91^0.03	0.244^0.003	0.4	1, 4
HD 105850	A1V	56.1	5.447^0.003	5.35^0.04	0.290^0.004	0.2	1, 2, 3, 4, 8, 22
HD 105912	F2/3V	50.0	6.940^0.007	5.96^0.06	0.258^0.004	2.7	1, 2, 3, 8, 23
HD 106906	F5V	59.0	7.798^0.008	6.76^0.04	0.184^0.003	0.015	1, 2, 3
HD 109573	A0V	67.1	5.777^0.004	5.79^0.04	0.231^0.003	0.01	2, 3, 4, 8, 22
HD 109704	A3V	68.8	5.869^0.003	5.77^0.05	0.245^0.003	0.4	1, 2, 3, 4, 8, 22
HD 112603	F2V	61.0	6.952^0.004	6.14^0.05	0.232^0.003	1.5	1, 6
HD 117716	A0/1V	72.0	5.690^0.004	5.67^0.03	0.255^0.003	0.3	1, 2, 3, 8
HD 118972	K1V	15.6	6.918^0.004	5.14^0.05	0.480^0.006	0.3	1, 2, 3, 7, 8, 11, 24
HD 136544	F6V	74.0	7.43^0.01	6.35^0.03	0.221^0.004	2.0	1, 9
HD 141378	A5IV	54.0	5.522^0.003	5.27^0.03	0.306^0.004	0.3	1, 2, 3, 8, 25
HD 141943	G0/2V	67.0	7.85^0.01	6.41^0.03	0.231^0.004	0.03	3, 8, 33
HD 142139	A3V	66.0	5.747^0.003	5.66^0.05	0.261^0.004	0.2	1, 2, 3, 4, 8
HD 161612	G6/8V	26.9	7.18^0.01	5.6^0.1	0.344^0.005	0.8	7, 11, 26
HD 174474	A2V	82.0	6.169^0.004	5.89^0.04	0.236^0.004	0.6	3, 4, 14, 15
HD 175073	K1V	24.0	7.96^0.01	5.95^0.03	0.324^0.005	4.1	1, 27
HD 178606	F5V	53.0	6.520^0.007	5.49^0.02	0.323^0.004	1.7	1, 23
HD 179520	F3V	62.0	7.092^0.007	6.24^0.02	0.232^0.003	0.6	1, 3, 23
HD 181327	F5/6V	52.0	7.035^0.008	5.98^0.04	0.263^0.004	0.021	1, 2, 3, 28, 31, 32
HD 184932	F2V	65.0	8.03^0.01	6.95^0.02	0.166^0.003	2.1	1, 4
HD 185615	G6IV	43.5	8.11^0.01	6.54^0.03	0.286^0.004	9.2	7, 9, 15
HD 191089	F5V	52.0	7.178^0.007	6.09^0.03	0.243^0.004	0.021	1, 3, 8, 22, 31, 32
HD 192758	F0V	62.0	7.013^0.008	6.30^0.04	0.217^0.004	0.04	3, 8, 29
HD 196141	G3V	37.0	8.09^0.01	6.58^0.03	0.213^0.004	0.4	7
HD 205674	F3/5IV	52.0	7.178^0.007	6.25^0.03	0.228^0.003	2.2	1, 3, 4, 8
HD 220476	G5V	30.0	7.611^0.009	6.11^0.04	0.276^0.004	0.4	7
HD 224228	K3V	22.0	8.237^0.009	6.01^0.03	0.325^0.005	0.1–0.2	1, 30

Notes. 1σ error bars are given as superscripts. V and H magnitudes are from Kharchenko & Roeser (2009). Limb-darkened stellar diameters (θ_LD) are computed from surface-brightness relationships based on the V and K magnitudes, following Kervella et al. (2004). References include previous searches for warm and cold dust around the target stars, with the reference in bold highlighting the origin of the warm dust classification that led to their addition to our sample, where applicable.

References. (1) Patel et al. (2014); (2) Ballering et al. (2013); (3) Cotten & Song (2016); (4) David & Hillenbrand (2015); (5) Bonfanti et al. (2016); (6) Holmberg et al. (2009); (7) Vican & Schneider (2014); (8) Chen et al. (2014); (9) Pace (2013); (10) Eiroa et al. (2013); (11) Valenti & Fischer (2005); (12) Delgado Mena et al. (2014); (13) Huensch et al. (1998); (14) Wu et al. (2013); (15) McDonald et al. (2012); (16) Durkan et al. (2016); (17) Tucci Maia et al. (2016); (18) Maldonado et al. (2012); (19) Desidera et al. (2015); (20) Pawellek et al. (2014); (21) Delgado Mena et al. (2015); (22) Mittal et al. (2015); (23) Feltzing et al. (2001); (24) Mamajek & Hillenbrand (2008); (25) De Rosa et al. (2014); (26) Tsantaki et al. (2013); (27) Casagrande et al. (2011); (28) Stark et al. (2014b); (29) Wahhaj et al. (2013); (30) Maire et al. (2014); (31) Zuckerman et al. (2004); (32) Binks & Jeffries (2014); (33) Chauvin et al. (2010).

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.