Skip to Main content Skip to Navigation
Journal articles

Multiwavelength study of the high-latitude cloud L1642: chain of star formation

Abstract : Context. L1642 is one of the two high galactic latitude (|b| > 30°) clouds confirmed to have active star formation.Aims. We examine the properties of this cloud, especially the large-scale structure, dust properties, and compact sources at different stages of star formation.Methods. We present high-resolution far-infrared and submillimetre observations with the Herschel and AKARI satellites and millimetre observations with the AzTEC/ASTE telescope, which we combined with archive data from near- and mid-infrared (2MASS, WISE) to millimetre wavelength observations (Planck).Results. The Herschel observations, combined with other data, show a sequence of objects from a cold clump to young stellar objects (YSOs) at different evolutionary stages. Source B-3 (2MASS J04351455-1414468) appears to be a YSO forming inside the L1642 cloud, instead of a foreground brown dwarf, as previously classified. Herschel data reveal striation in the diffuse dust emission around the cloud L1642. The western region shows striation towards the NE and has a steeper column density gradient on its southern side. The densest central region has a bow-shock like structure showing compression from the west and has a filamentary tail extending towards the east. The differences suggest that these may be spatially distinct structures, aligned only in projection. We derive values of the dust emission cross-section per H nucleon of σe(250 μm) = 0.5−1.5 × 10-25 cm2/H for different regions of the cloud. Modified black-body fits to the spectral energy distribution of Herschel and Planck data give emissivity spectral index β values 1.8–2.0 for the different regions. The compact sources have lower β values and show an anticorrelation between T and β.Conclusions. Markov chain Monte Carlo calculations demonstrate the strong anticorrelation between β and T errors and the importance of millimetre wavelength Planck data in constraining the estimates. L1642 reveals a more complex structure and sequence of star formation than previously known.
Document type :
Journal articles
Complete list of metadata

Cited literature [46 references]  Display  Hide  Download
Contributor : Edp Sciences <>
Submitted on : Thursday, November 26, 2015 - 6:00:06 PM
Last modification on : Monday, April 5, 2021 - 2:26:14 PM
Long-term archiving on: : Saturday, April 29, 2017 - 12:25:34 AM


Publication funded by an institution



J. Malinen, M. Juvela, S. Zahorecz, A. Rivera-Ingraham, J. Montillaud, et al.. Multiwavelength study of the high-latitude cloud L1642: chain of star formation. Astronomy and Astrophysics - A&A, EDP Sciences, 2014, 563, pp.A125. ⟨10.1051/0004-6361/201323026⟩. ⟨cea-01234368⟩



Record views


Files downloads