( en | de | ru )

 

Disambiguierung von "Madden, Suzanne"

Autor der Publikation

KopierenLöschenDiese Publikation zur Ablage hinzufügen
Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud

, , , , , , , , , , , , , , , , , , , , , , und . (2014)cite arxiv:1407.7658Comment: Submitted to MNRAS.

Bitte wählen Sie eine Person um die Publikation zuzuordnen

Um zwischen Personen mit demselben Namen zu unterscheiden, wird der akademische Grad und der Titel einer wichtigen Publikation angezeigt. Zudem lassen sich über den Button neben dem Namen einige der Person bereits zugeordnete Publikationen anzeigen.

Neil Madden

Peter Madden

Suzanne Bontemps

Suzanne Perz

Suzanne Adang

 

Weitere Publikationen von Autoren mit dem selben Namen

Radiative and mechanical feedback into the molecular gas in the Large Magellanic Cloud. II. 30 Doradus, , , , , , , , und . (2019)cite arxiv:1905.10051Comment: Accepted for publication in A&A.The Herschel Virgo Cluster Survey. IX. Dust-to-gas mass ratio and metallicity gradients in four Virgo spiral galaxies, , , , , , , , , und 13 andere Autor(en). (2011)cite arxiv:1106.0618Comment: 13 pages, 8 figures, A&A accepted.Molecular hydrogen emission in the interstellar medium of the Large Magellanic Cloud, , , , , , , , , und 13 andere Autor(en). (2014)cite arxiv:1407.7658Comment: Submitted to MNRAS.The Illusive ISM of Dwarf Galaxies: Excess Submillimetre Emission and CO-Dark Molecular Gas, , , , , , , , , und 7 andere Autor(en). (2011)cite arxiv:1105.1006 Comment: Proceedings of the 5th Zermatt Symposium: "Conditions and Impact of Star Formation: New Results from Herschel and Beyond" September 19-24, 2010.The State of the Gas and the Relation Between Gas and Star Formation at Low Metallicity: the Small Magellanic Cloud, , , , , , , , , und 8 andere Autor(en). (2011)cite arxiv:1107.1717Comment: Accepted for publication in the Astrophysical Journal. 21 pages and 11 figures in apjemulate style.The Herschel Virgo Cluster Survey: X.The relationship between cold dust and molecular gas content in Virgo spirals, , , , , , , , , und 9 andere Autor(en). (2012)cite arxiv:1204.4628Comment: 11 pages, 8 figures. Accepted for publication in A&A.The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds, , , , , , , , , und 7 andere Autor(en). (2015)cite arxiv:1510.08084Comment: 24 pages, 14 figures, submitted for publication in ApJ.Observations of Arp 220 using Herschel-SPIRE: An Unprecedented View of the Molecular Gas in an Extreme Star Formation Environment, , , , , , , , , und 13 andere Autor(en). (2011)cite arxiv:1106.5054Comment: submitted to ApJ June 13, 2011.Measuring the HI content of individual galaxies out to the epoch of reionization with CII, , , , und . (2021)cite arxiv:2108.13442Comment: Accepted for publication in ApJ.Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview, , , , , , , , , und 50 andere Autor(en). (2011)cite arxiv:1107.4313Comment: 16 pages, 11 figures, AJ, in press.