Astrochemical confirmation of the rapid evolution of massive YSOs and explanation for the inferred ages of hot cores

E-ISSN： 1432-0746|454|1|L5-L8

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.454, Iss.1, 2006-07, pp. : L5-L8

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Evolution of complex organic molecules in hot molecular cores

By Choudhury R. Schilke P. Stéphan G. Bergin E. Möller T. Schmiedeke A. Zernickel A.

Astronomy & Astrophysics, Vol. 575, Iss. issue, 2015-02 ,pp. : A68-A68

Edp Sciences

Access to resources Recommend Favorite

Collective pulsational velocity broadening due to gravity modes as a physical explanation for macroturbulence in hot massive stars

Astronomy & Astrophysics, Vol. 508, Iss. 1, 2009-12 ,pp. : 409-419

Edp Sciences

Access to resources Recommend Favorite

The RMS survey: mid-infrared observations of candidate massive YSOs in the southern hemisphere

Astronomy & Astrophysics, Vol. 476, Iss. 2, 2007-12 ,pp. : 1019-1111

Edp Sciences

Access to resources Recommend Favorite

VLT/ISAAC H-band spectroscopy of embedded massive YSOs

Astronomy & Astrophysics, Vol. 408, Iss. 1, 2003-09 ,pp. : 313-322

Edp Sciences

Access to resources Recommend Favorite

The Deuteration Clock for Massive Starless Cores

EAS Publications Series, Vol. 75-76, Iss. issue, 2016-05 ,pp. : 337-341

Edp Sciences

Access to resources Recommend Favorite