EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 573 (January 2015) A&A, 573 (2015) A97 Full HTML
Free Access

Table A.1

Diffuse interstellar bands in Tc 1 and HR 6334.

Tc 1 HR 6334
λ c Components FWHM EQW S/N EQW/E B − V λc Components FWHM EQW S/N EQW/E B − V
(Å) (Å) (Å) (mÅ) (Å/mag) (Å) (Å) (Å) (mÅ) (Å/mag)
4427.51ab ... 19.35 860.0 403 3.74 4429.71 ... 23.42 470.2 391 1.12
5776.22 ... 1.14 7.2 402 0.03 5776.11 ... 1.21 5.3 535 0.01
5780.65b ... 2.02 112.1 420 0.49 5780.59 ... 2.17 119.0 586 0.28
5797.21 ... 0.82 25.7 536 0.11 5797.19 ... 1.15 45.7 590 0.11
5849.74 ... 0.89 2.2 437 0.01 5849.74 ... 0.76 12.7 536 0.03
6196 6196.06c 1.11 10.7 525 0.05 6196 6196.05c 0.96 16.0 692 0.04
6195.88 0.48 6.0 0.03 6195.89 0.40 10.4 0.02
6196.54 0.39 2.6 0.01 6196.56 0.36 4.3 0.01
6203.33 ... 2.03 36.7 560 0.16 6203.17 ... 1.28 29.1 758 0.07
6250.36 ... 1.74 8.7 610 0.04 6250.62 ... 2.45 14.7 727 0.03
6270.08 ... 1.66 15.0 618 0.06 6270 6269.98 1.47 25.8 494 0.06
6284.18 ... 4.41 630 380 1.66 6284.15 ... 4.55 309.8 693 0.74
6376 6376.22c 1.38 2.6 559 0.01 6376 6376.40c 1.36 12.7 612 0.03
6376.05 0.57 1.7 0.01 6375.92 0.41 3.6 0.01
6376.76 0.48 1.6 0.01 6376.65 0.76 6.4 0.01
6379 6379.41c 1.13 8.7 625 0.04 6379 6379.47c 1.26 56.4 812 0.13
6379.14 0.56 4.9 0.02 6379.14 0.46 21.0 0.05
6379.82 0.93 4.7 0.02 6379.78 1.08 35.4 0.08
6597.18 ... 0.48 4.1 529 0.02 6597.14 ... 0.45 5.0 338 0.01
6613.77 ... 1.47 32.5 432 0.14 6613.74 ... 1.40 91.8 464 0.22
6661 6661.09c 1.12 3.5 341 0.01 6661 6660.81c 1.09 22.8 337 0.05
6660.64 0.64 2.5 0.01 6660.61 0.54 14.4 0.03
6661.40 0.24 1.9 0.01 6661.35 0.30 5.4 0.01
6792.22 ... 1.16 12.6 360 0.05 6792.07 ... 1.10 15.2 329 0.04
7828.75 ... 1.49 8.8 382 0.04 7828.45 ... 1.07 6.1 572 0.01
7832.50 ... 1.76 10.3 475 0.04 7832.63 ... 2.11 14.5 636 0.03
8038.14 ... 0.96 5.4 396 0.02 8038.01 ... 0.81 7.0 460 0.02
8621.12 ... 4.52 63.4 348 0.28 8621.15 ... 4.50 51.7 626 0.12

Notes. The 3σ errors in the EQWs scale as ~3 ×FWHM/(S/N), while we estimate that the FHWMs in Tc 1 are precise to the 0.03 Å level (less for M 1-20 and IC 418).

(a)

The parameters of this DIB are estimated by adopting a Lorentzian profile (see, e.g., Snow et al. 2002).

(b)

Circumstellar absorption features (or diffuse circumstellar bands) may be possibly detected at these wavelengths (see Sect. 4).

(c)

Undeblended DIB.

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.