The resolved star formation history of M51a through successive Bayesian marginalization-Reference-Cited by-同舟云学术

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The resolved star formation history of M51a through successive Bayesian marginalization

Published:2017-10-27 Issue:2 Volume:474 Page:1862-1872
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Martínez-García Eric E.,Bruzual Gustavo,Magris C. Gladis,González-Lópezlira Rosa A.

Funder

UNAM

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/474/2/1862/22637162/stx2801.pdf

Reference69 articles.

1. Understanding the scatter in the spatially resolved star formation main sequence of local massive spiral galaxies

2. THE ELEVENTH AND TWELFTH DATA RELEASES OF THE SLOAN DIGITAL SKY SURVEY: FINAL DATA FROM SDSS-III

3. Common-Resolution Convolution Kernels for Space- and Ground-Based Telescopes

4. The star cluster population of M 51

5. THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROMz= 0-8

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1. On the Thermally Pulsing Asymptotic Giant Branch Contribution to the Light of Nearby Disk Galaxies;The Astrophysical Journal;2021-02-01

2. Late Bloomer Galaxies: Growing Up in Cosmic Autumn;The Astrophysical Journal;2018-12-20

3. Approximations to galaxy star formation rate histories: properties and uses of two examples;Monthly Notices of the Royal Astronomical Society;2018-05-03

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