Related content

Gas-phase CO$_\mathsf{2}$, C$_\mathsf{2}$H$_\mathsf{2}$, and HCN toward Orion-KL

By  

Astronomy & Astrophysics, Vol. 399, Iss. 3, 2003-03 ,pp. : 1047-1061

Edp Sciences

Access to resources Recommend Favorite

H$_{\mathsf 2}$CO and CH$_{\mathsf 3}$OH maps of the Orion Bar photodissociation region*

By Leurini S.   Parise B.   Schilke P.   Pety J.   Rolffs R.  

Astronomy & Astrophysics, Vol. 511, Iss. issue, 2010-03 ,pp. : A82-A82

Edp Sciences

Access to resources Recommend Favorite

Observational 2D model of H$\mathsf{_2}$ emission from a bow shock in the Orion Molecular Cloud

By  

Astronomy & Astrophysics, Vol. 477, Iss. 1, 2008-01 ,pp. : 203-211

Edp Sciences

Access to resources Recommend Favorite

H$\mathsf{_2}$ infrared emission and the formation of dense structures in the Orion molecular cloud

By  

Astronomy & Astrophysics, Vol. 366, Iss. 2, 2001-02 ,pp. : 651-661

Edp Sciences

Access to resources Recommend Favorite

Theoretical H$_\mathsf{2}$CO emission from protostellar envelopes

By  

Astronomy & Astrophysics, Vol. 410, Iss. 2, 2003-11 ,pp. : 587-595

Edp Sciences

Access to resources Recommend Favorite