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An interesting nebular object in LDN 288
(SPRINGER/PLENUM PUBLISHERS, 2006-10)
In this paper the results of multiwavelength investigation of an unusual nebular object SNO 85 are presented. In 2MASS images this object looks like a star with a jet. In DSS2 R image the end of the jet is connected with ...
Modelling the spinning dust emission from LDN1780
(Oxford University Press, 2020)
We study the anomalous microwave emission (AME) in the Lynds Dark Nebula (LDN) 1780 on two angular scales. With publicly available data at an angular resolution of 1 degrees, we studied the spectral energy distribution of ...
Dust-correlated centimetre-wave radiation from the M78 reflection nebula
(2011)
An anomalous radio continuum component at cm-wavelengths has been observed in various sources, including dark clouds. This continuum component represents a new property of the ISM. In this work we focus on one particular ...
An X-ray study of the supernova remnant G20.0-0.2 and its surroundings
(Edp Sciences, 2013-06)
Aims. We study the supernova remnant G20.0-0.2 and its surroundings in order to look for the high energy counterpart of the radio nebula and to find evidence of interaction between the shock front and the interstellar ...
Dust-correlated centimetre-wave radiation from the M78 reflection nebula
(2011)
An anomalous radio continuum component at cm-wavelengths has been observed in various sources, including dark clouds. This continuum component represents a new property of the ISM. In this work we focus on one particular ...
Unveiling a cluster of protostellar disks around the massive protostar GGD 27 MM1
(EDP Sciences, 2019-03)
Context. Most stars form in clusters and thus it is important to characterize the protostellar disk population in dense environments to assess whether the environment plays a role in the subsequent evolution. Specifically, ...
Dust-correlated centimetre-wave radiation from the M78 reflection nebula
(WILEY-BLACKWELL, 2011-02)
An anomalous radio continuum component at cm-wavelengths has been observed in
various sources, including dark clouds. This continuum component represents a new
property of the ISM. In this work we focus on one particular ...
A new study of the supernova remnant G344.7-0.1 located in the vicinity of the unidentified TeV source HESS J1702-420
(EDP Sciences, 2011-07)
Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understanding of their underlying astrophysical processes.
Aims. We investigate the physical properties of the supernova remnant ...