Cite
The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period–Luminosity Relations
MLA
Shu Wang, et al. “The Near-Infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-Infrared Period–Luminosity Relations.” The Astrophysical Journal, vol. 852, Jan. 2018, p. 78. EBSCOhost, widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi.dedup.....83d2c60fe28bde6156689e3eac8a42e6&authtype=sso&custid=ns315887.
APA
Shu Wang, Licai Deng, Xiaodian Chen, & Richard de Grijs. (2018). The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period–Luminosity Relations. The Astrophysical Journal, 852, 78.
Chicago
Shu Wang, Licai Deng, Xiaodian Chen, and Richard de Grijs. 2018. “The Near-Infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-Infrared Period–Luminosity Relations.” The Astrophysical Journal 852 (January): 78. http://widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi.dedup.....83d2c60fe28bde6156689e3eac8a42e6&authtype=sso&custid=ns315887.