Spectra of 7 H{alpha} emission line stars in MBM 18 Virtual Observatory Resource

Authors

1. Brand J.
2. Wouterloot J.G.A.
3. Magnani L.

Published by

CDS

Abstract

We investigate star formation in translucent, high-latitude clouds. Our aim is to understand the star-formation history and rate in the solar neighbourhood. We used spectroscopic observations of newly found candidate H{alpha} emission-line stars to establish their pre-main-sequence nature. The environment was studied through molecular line observations of the cloud (MBM 18/LDN 1569) in which the stars are presumably embedded.

Keywords

1. molecular-clouds
2. emission-line-stars
3. spectroscopy

Bibliographic source Bibcode

2012A&A...547A..85B

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IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/547/A85

Document Object Identifer DOI

doi:10.26093/cds/vizier.35470085

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