Exploring the connection between stellar halo profiles and accretion histories in L _* galaxies

E-ISSN： 1743-9221|11|S321|90-92

ISSN： 1743-9213

Source： Proceedings of the International Astronomical Union, Vol.11, Iss.S321, 2017-03, pp. : 90-92

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

Abstract

Related content

Evolution of the anti-truncated stellar profiles of S0 galaxies since z=0.6 in the SHARDS survey

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 280-280

Cambridge University Press

Access to resources Recommend Favorite

No direct coupling between bending of galaxy disc stellar age and light profiles as seen from CALIFA

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 278-278

Cambridge University Press

Access to resources Recommend Favorite

The halo-to-stellar mass ratio in the S⁴G

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 281-281

Cambridge University Press

Access to resources Recommend Favorite

Stellar populations in the highest redshift galaxies

Proceedings of the International Astronomical Union, Vol. 11, Iss. A29B, 2016-10 ,pp. : 197-198

Cambridge University Press

Access to resources Recommend Favorite

Accretion phenomena in nearby star-forming dwarf galaxies

Proceedings of the International Astronomical Union, Vol. 11, Iss. S321, 2017-03 ,pp. : 211-213

Cambridge University Press

Access to resources Recommend Favorite