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Jump to: 2022 | 2020 | 2015
Number of items: 4.

2022

Schneider, N., Ossenkopf-Okada, V, Clarke, S., Klessen, R. S., Kabanovic, S., Veltchev, T., Bontemps, S., Dib, S., Csengeri, T., Federrath, C., Di Francesco, J., Motte, F., Andre, Ph, Arzoumanian, D., Beattie, J. R., Bonne, L., Didelon, P., Elia, D., Konyves, V, Kritsuk, A., Ladjelate, B., Myers, Ph, Pezzuto, S., Robitaille, J. F., Roy, A., Seifried, D., Simon, R., Soler, J. and Ward-Thompson, D. (2022). Understanding star formation in molecular clouds IV. Column density PDFs from quiescent to massive molecular clouds. Astron. Astrophys., 666. LES ULIS CEDEX A: EDP SCIENCES S A. ISSN 1432-0746

2020

Ladjelate, B., Andre, Ph, Konyves, V, Ward-Thompson, D., Men'shchikov, A., Bracco, A., Palmeirim, P., Roy, A., Shimajiri, Y., Kirk, J. M., Arzoumanian, D., Benedettini, M., Di Francesco, J., Fiorellino, E., Schneider, N., Pezzuto, S. and Motte, F. (2020). The Herschel view of the dense core population in the Ophiuchus molecular cloud. Astron. Astrophys., 638. LES ULIS CEDEX A: EDP SCIENCES S A. ISSN 1432-0746

Zavagno, A., Andre, Ph, Schuller, F., Peretto, N., Shimajiri, Y., Arzoumanian, D., Csengeri, T., Figueira, M., Fuller, G. A., Konyves, V, Men'shchikov, A., Palmeirim, P., Roussel, H., Russeil, D., Schneider, N. and Zhang, S. (2020). The role of Galactic HII regions in the formation of filaments: High-resolution submilimeter imaging of RCW 120 with ArTeMiS. Astron. Astrophys., 638. LES ULIS CEDEX A: EDP SCIENCES S A. ISSN 1432-0746

2015

Schneider, N., Bontemps, S., Girichidis, P., Rayner, T., Motte, F., Andre, Ph, Russeil, D., Abergel, A., Anderson, L., Arzoumanian, D., Benedettini, M., Csengeri, T., Didelon, P., Di Francesco, J., Griffin, M., Hill, T., Klessen, R. S., Ossenkopf, V., Pezzuto, S., Rivera-Ingraham, A., Spinoglio, L., Tremblin, P. and Zavagno, A. (2015). Detection of two power-law tails in the probability distribution functions of massive GMCs. Mon. Not. Roy. Astron. Soc., 453 (1). S. L41 - 5. OXFORD: OXFORD UNIV PRESS. ISSN 1365-2966

This list was generated on Thu Nov 28 13:59:58 2024 CET.