On the origin of the system PSR B 1757$\mathsf{-}$24/SNR G 5.4$\mathsf{-}$1.2

E-ISSN： 1432-0746|415|3|1073-1078

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.415, Iss.3, 2004-03, pp. : 1073-1078

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

Polarization observations of SNR G156.2+5.7 at $\mathsf{\lambda}$6 cm

Astronomy & Astrophysics, Vol. 470, Iss. 3, 2007-08 ,pp. : 969-975

Edp Sciences

Access to resources Recommend Favorite

The gravitational collapse of ONe electron-degenerate cores and white dwarfs: The role of $^\mathsf{24}$Mg and $^\mathsf{12}$C revisited

Astronomy & Astrophysics, Vol. 435, Iss. 1, 2005-05 ,pp. : 231-237

Edp Sciences

Access to resources Recommend Favorite

PSR B 1706-44 and the SNR G 343.1-2.3 as the remnants of a cavity supernova explosion

Astronomy & Astrophysics, Vol. 394, Iss. 2, 2002-11 ,pp. : 533-538

Edp Sciences

Access to resources Recommend Favorite

The stellar origin of $\mathsf{^7}$Li

Astronomy & Astrophysics, Vol. 374, Iss. 2, 2001-08 ,pp. : 646-655

Edp Sciences

Access to resources Recommend Favorite

The 12 $\mathsf{\mu}$m ISO-ESO-Sculptor and 24 $\mathsf{\mu}$m Spitzer faint counts reveal a population of ULIRGs as dusty massive ellipticals

Astronomy & Astrophysics, Vol. 475, Iss. 3, 2007-12 ,pp. : 801-812

Edp Sciences

Access to resources Recommend Favorite