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

DOI

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.

Cone search capability for table J/A+A/547/A85/table1 (Coordinates and magnitudes of the candidate H{alpha} emission-line stars, and log of TNG observations)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35470085
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/547/A85
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/547/A85
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/547/A85
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/547/A85
Provenance
Creator Brand J.; Wouterloot J.G.A.; Magnani L.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Interstellar medium; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy