A new spectroscopic and interferometric study of the young stellar object V645 Cygni

A. S. Miroshnichenko; K.-H. Hofmann; D. Schertl; G. Weigelt; S. Kraus; N. Manset; L. Albert; Y. Y. Balega; V. G. Klochkova; R. J. Rudy; D. K. Lynch; S. Mazuk; C. C. Venturini; R. W. Russell; K. N. Grankin; R. C. Puetter; R. B. Perry

doi:10.1051/0004-6361/200810936

Home

All issues

Volume 498 / No 1 (April IV 2009)

A&A, 498 1 (2009) 115-126

Full HTML

Free Access

Table 1:

Published results for the nature and evolutionary state of V645 Cyg.
Sp.	A_V	V	D	Ref.
type	mag	mag	kpc
O7	4.2	15.1^a	$\ge$ 3, $\sim$ 6	Cohen (1977)
	3.6		$\ge$ 1, $\le$ 6	Humphreys et al. (1980)
A0	2.5		3.5 $\pm$ 0.5	Goodrich (1986)

Estimate of the star's spectral type is listed in Col. 1; interstellar extinction toward the object in Col. 2; object's visual brightness in Col. 3; distance toward the object in Col. 4; and a reference to the estimates in Col. 5; ^a the brightness for the knot N0.

Source LaTeX | All tables | In the text

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.