Scattered H-alpha emission from a large translucent cloud G294-24

Abstract

We study an undocumented large translucent cloud, detected by means of its enhanced radiation on the SHASSA (Southern H-Alpha Sky Survey Atlas) survey. We consider whether its excess surface brightness can be explained by light scattered off the dust grains in the cloud, or whether emission from in situ ionized gas is required. In addition, we aim to determine the temperature of dust, the mass of the cloud, and its possible star formation activity. We compare the observed H-alpha surface brightness of the cloud with predictions of a radiative transfer model. We use the WHAM (Wisconsin H-Alpha Mapper) survey as a source for the Galactic H-alpha interstellar radiation field illuminating the cloud. Visual extinction through the cloud is derived using 2MASS J, H, and K band photometry. We use far-IR ISOSS (ISO Serendipitous Survey), IRAS, and DIRBE data to study the thermal emission of dust. The LAB (The Leiden/Argentine/Bonn Galactic HI Survey) is used to study 21cm HI emission associated with the cloud. Radiative transfer calculations of the Galactic diffuse H-alpha radiation indicate that the surface brightness of the cloud can be explained solely by radiation scattered off dust particles in the cloud. The maximum visual extinction through the cloud is about 1.2mag. The cloud is found to be associated with 21cm HI emission at a velocity of about -9 km/s. The total mass of the cloud is about 550-1000 solar masses. There is no sign of star formation in this cloud. The distance of the cloud is estimated from the Hipparcos data to be about 100 pc.

References in corpus (7)

• The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
• IRIS: A new generation of IRAS maps
• A high sensitivity HI survey of the sky at delta < -25 deg Final data release
• Efficient Monte Carlo methods for continuum radiative transfer
• ISO far infrared observations of the high latitude cloud L1642. II. Correlated variations of far-infrared emissivity and temperature of "classical large" dust particles
• Unresolved H-Alpha Enhancements at High Galactic Latitude in the WHAM Sky Survey Maps
• Properties of dust and detection of Halpha emission in LDN 1780

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• Spectroscopy of diffuse light in dust clouds. Scattered light and the solar neighbourhood radiation field
• Shaken or stirred: the diffuse interstellar medium with exceptionally high SiO abundance
• A Monte Carlo Implementation of Galactic Free-Free Emission for the EoR Foreground Models