Dense cores in the dark cloud complex LDN 1188

E. Verebélyi, V. Könyves, S. Nikolić, C. Kiss, A. Moór, P. Äbrahám, M. Kun

Research output: Contribution to journalArticle

3 Citations (Scopus)

Abstract

We present a molecular line emission study of the LDN 1188 dark cloud complex located in Cepheus. In this work we focused on the densest parts of the cloud and on the close neighbourhood of infrared point sources. We made ammonia mapping with the Effelsberg 100 m radio telescope and identified 3 dense cores. CS(1-0), CS(2-1) and HCO+(1-0) measurements performed with the Onsala 20 m telescope revealed the distribution of dense molecular material. The molecular line measurements were supplemented by mapping the dust emission at 1.2 mm in some selected directions using the IRAM 30 m telescope. With these data we could work out a likely evolutionary sequence in this dark cloud complex.

Original languageEnglish
Pages (from-to)920-923
Number of pages4
JournalAstronomische Nachrichten
Volume334
Issue number9
DOIs
Publication statusPublished - Nov 2013

Keywords

  • ISM: clouds
  • ISM: individual (LDN 1188)
  • ISM: molecules
  • Radio lines: ISM

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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