2013A&A...549A..91L


C.D.S. - SIMBAD4 rel 1.7 - 2021.05.05CEST23:27:58

2013A&A...549A..91L - Astronomy and Astrophysics, volume 549A, 91-91 (2013/1-1)

Spectroscopy of diffuse light in dust clouds. Scattered light and the solar neighbourhood radiation field.

LEHTINEN K. and MATTILA K.

Abstract (from CDS):

The optical surface brightness of dark nebulae is mainly due to scattering of integrated starlight by classical dust grains. It contains information on the impinging interstellar radiation field, cloud structure, and grain scattering properties. We have obtained spectra of the scattered light from 3500 to 9000Å in two globules, the Thumbprint Nebula and DC 303.8-14.2. We use observations of the scattered light to study the impinging integrated starlight spectrum as well as the scattered Hα and other line emissions from all over the sky. We search also for the presence of other than scattered light in the two globules. We obtained long-slit spectra encompassing the whole globule plus adjacent sky in a one-slit setting, thus enabling efficient elimination of airglow and other foreground sky components. We calculated synthetic integrated starlight spectra for the solar neighbourhood using Hipparcos-based stellar distributions and the spectral library of Pickles. Spectra are presented separately for the bright rims and dark cores of the globules. The continuum spectral energy distributions and absorption line spectra can be well modelled with the synthetic integrated starlight spectra. Emission lines of Hα+[NII], Hβ, and [SII] are detected and are interpreted in terms of scattered light plus an in situ warm ionized medium component behind the globules. We detected an excess of emission over the wavelength range 5200-8000Å in DC 303.8-14.2 but the nature of this emission remains open.

Abstract Copyright:

Journal keyword(s): ISM: clouds - ISM: lines and bands - dust, extinction - solar neighborhood - radiative transfer - methods: observational

Simbad objects: 10

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Number of rows : 10

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 LDN 1642 MoC 04 35 18 -14 13.9           ~ 140 0
2 LP 673-37 PM* 11 45 14.2114223648 -09 28 24.560105740     13.84     ~ 6 0
3 LAWD 37 WD* 11 45 42.9170659451 -64 50 29.464090822 11.08 11.725 11.513 11.34 11.163 DQ 238 0
4 NAME Chamaeleon Region SFR 11 55 -78.0           ~ 712 0
5 IRAS 12340-7958 * 12 37 39.7466355997 -80 15 13.713429632   16.11 14.39 13.63 9.81 ~ 101 0
6 NAME Cha III MoC 12 37.8 -80 15           ~ 132 2
7 BHR 84 MoC 12 44 35 -78 48.2           ~ 9 0
8 NAME Thumbprint Nebula DNe 12 44 55.6 -78 48 16           ~ 22 0
9 Sandqvist 160 DNe 13 06.9 -77 01           ~ 41 0
10 LDN 1780 DNe 15 39.7 -07 10           ~ 73 0

    Equat.    Gal    SGal    Ecl

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2021.05.05-23:27:58

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