Philipp Podsiadlowski: Publications

No surviving non-compact stellar companion to Cassiopeia A

ASTRONOMY & ASTROPHYSICS 623 (2019) ARTN A34

Authors:

Wolfgang E Kerzendorf, Tuan Do, Selma E de Mink, Ylva Gotberg, Dan Milisavljevic, Emmanouil Zapartas, Mathieu Renzo, Stephen Justham, Philipp Podsiadlowski, Robert A Fesen

On the formation history of Galactic double neutron stars

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 481:3 (2018) 4009-4029

Authors:

Alejandro Vigna-Gomez, Coenraad J Neijssel, Simon Stevenson, Jim W Barrett, Krzysztof Belczynski, Stephen Justham, Selma E de Mink, Bernhard Mueller, Philipp Podsiadlowski, Mathieu Renzo, Dorottya Szecsi, Ilya Mandel

Comprehensive 51�� of Ejecta-companion Interaction for Core-collapse Supernovae in Massive Binaries

ASTROPHYSICAL JOURNAL 864:2 (2018) ARTN 119

Authors:

Ryosuke Hirai, Philipp Podsiadlowski, Shoichi Yamada

Do SN 2002cx-like and SN Ia-CSM Objects Share the Same Origin?

ASTROPHYSICAL JOURNAL 861:2 (2018) ARTN 127

Authors:

X Meng, Ph Podsiadlowski

Response to Comment on "An excess of massive stars in the local 30 Doradus starburst".

Science (New York, N.Y.) 361:6400 (2018)

Authors:

Fabian RN Schneider, Hugues Sana, Christopher J Evans, Joachim M Bestenlehner, Norberto Castro, Luca Fossati, Götz Gräfener, Norbert Langer, Oscar H Ramírez-Agudelo, Carolina Sabín-Sanjulián, Sergio Simón-Díaz, Frank Tramper, Paul A Crowther, Alexander de Koter, Selma E de Mink, Philip L Dufton, Miriam Garcia, Mark Gieles, Vincent Hénault-Brunet, Artemio Herrero, Robert G Izzard, Venu Kalari, Danny J Lennon, Jesús Maíz Apellániz, Nevy Markova, Francisco Najarro, Philipp Podsiadlowski, Joachim Puls, William D Taylor, Jacco Th van Loon, Jorick S Vink, Colin Norman

Abstract:

Farr and Mandel reanalyze our data, finding initial mass function slopes for high-mass stars in 30 Doradus that agree with our results. However, their reanalysis appears to underpredict the observed number of massive stars. Their technique results in more precise slopes than in our work, strengthening our conclusion that there is an excess of massive stars (>30 solar masses) in 30 Doradus.

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