The Planck submillimeter properties of Galactic high-mass star forming regions: dust temperatures, luminosities, masses and Star Formation Efficiency

MLA

Paladini, R., et al. The Planck Submillimeter Properties of Galactic High-Mass Star Forming Regions: Dust Temperatures, Luminosities, Masses and Star Formation Efficiency. 2021. EBSCOhost, https://doi.org/10.3847/1538-4357/abe711.

APA

Paladini, R., Mottram, J. C., Veneziani, M., Traficante, A., Schisano, E., Giardino, G., Falgarone, E., Urquhart, J. S., Harrison, D. L., Joncas, G., Umana, G., & Molinari, S. (2021). The Planck submillimeter properties of Galactic high-mass star forming regions: dust temperatures, luminosities, masses and Star Formation Efficiency. https://doi.org/10.3847/1538-4357/abe711

Chicago

Paladini, R., J. C. Mottram, M. Veneziani, A. Traficante, E. Schisano, G. Giardino, E. Falgarone, et al. 2021. “The Planck Submillimeter Properties of Galactic High-Mass Star Forming Regions: Dust Temperatures, Luminosities, Masses and Star Formation Efficiency.” doi:10.3847/1538-4357/abe711.