Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Eric W. Pellegrini"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 520:5600-5612
We study the evolution of embedded star clusters with the goal to reproduce 30 Doradus, specifically the compact star cluster known as R136 and its surrounding stellar envelope, which is believed to be part of an earlier star formation event. We empl
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 492(1), 915-933. Oxford University Press
We explore to what extent simple algebraic models can be used to describe H II regions when winds, radiation pressure, gravity and photon breakout are included. We a) develop algebraic models to describe the expansion of photoionised H II regions und
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 483:2547-2560
Star formation is an inefficient process and in general only a small fraction of the gas in a giant molecular cloud (GMC) is turned into stars. This is partly due to the negative effect of stellar feedback from young massive star clusters. In a recen
Autor:
Suzanne Ramsay, J. M. D. Kruijssen, Leonardo Testi, Chris Evans, Eric W. Pellegrini, Adam Ginsburg, A. F. McLeod, James E. Dale
Publikováno v:
Monthly Notices of the Royal Astronomical Society
We present MUSE integral field data of two HII region complexes in the Large Magellanic Cloud (LMC), N44 and N180. Both regions consist of a main superbubble and a number of smaller, more compact HII regions that formed on the edge of the superbubble
Autor:
Daniel Rahner, A. Werle, Simon C. O. Glover, Ralf S. Klessen, A. L. de Amorim, Benjamin D. Johnson, Vivienne Wild, R. C. Kennicutt, Eric W. Pellegrini, Yirui Zheng, Stefan Reissl, Maud Galametz, N. Vale Asari
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The H$\alpha$ and H$\beta$ emission line luminosities measured in a single integrated spectrum are affected in non-trivial ways by point-to-point variations in dust attenuation in a galaxy. This work investigates the impact of this variation when est
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::935971e95ae77e021d0f6df31cf74033
http://adsabs.harvard.edu/abs/2020arXiv200705544V
http://adsabs.harvard.edu/abs/2020arXiv200705544V
Autor:
Mark Wolfire, J. D. T. Smith, Elias Brinks, Eric J. Murphy, Eric W. Pellegrini, Lee Armus, Eva Schinnerer, Leslie K. Hunt, Daniel A. Dale, Bruce T. Draine, Christine D. Wilson, Rodrigo Herrera-Camus, Karin Sandstrom, Alison F. Crocker, Robert C. Kennicutt, Dimitra Rigopoulou, Brent Groves, Erik Rosolowsky, Paul van der Werf
Publikováno v:
University of Hertfordshire
Astrophysical Journal (0004-637X), 887(1), 105
Astrophysical Journal (0004-637X), 887(1), 105
We present resolved [CI] line intensities of 18 nearby galaxies observed with the SPIRE FTS spectrometer on the Herschel Space Observatory. We use these data along with resolved CO line intensities from $J_\mathrm{up} = 1$ to 7 to interpret what phas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37b4f56420a93a2d5de1c898ab045a8f
https://doi.org/10.3847/1538-4357/ab4196
https://doi.org/10.3847/1538-4357/ab4196
Autor:
Roberto Cid Fernandes, M. Girard, A. Luiz de Amorim, I. Millan, Martin Bureau, P. Amram, Eric W. Pellegrini, Gilles Joncas, Anne Pellerin, Francoise Combes, Hugo Martel, Julie Hlavacek-Larrondo, Dimitrios A. Gouliermis, B. Mazzilli-Ciraulo, Thomas Martin, Jorge Iglesias-Páramo, Christophe Morisset, Andreea Petric, S. Duarte Puertas, Marianne Takamiya, Rieko Momose, T. Ruiz Lara, Pauline Barmby, A. F. McLeod, I-Ting Ho, Fumi Egusa, Laurie Rousseau-Nepton, Ralf S. Klessen, Benoît Epinat, Mercedes Mollá, Angela Adamo, C. Robert, Isabel Pérez, Alexandre Alarie, A. K. Pati, Alessandro Boselli, Laurent Chemin, Grazyna Stasinska, L. Sánchez-Menguiano, Lijie Liu, Simon Prunet, Zacharie Sie Kam, Victor F. Ksoll, Kathryn Grasha, Clare Higgs, J. D. Lyman, Q. Liu, L. Della Bruna, Henri Plana, I. Moumen, N. Vale Asari, V. Gómez Llanos, Daniel Rahner, Hsi-An Pan, Fabio Bresolin, Anne-Laure Melchior, Laurent Drissen, José M. Vílchez, Robert C. Kennicutt, Kristine Spekkens, C. Crowder, R. P. Martin, Sophia Lianou, P. Karera
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 489 (4), pp.5530-5546. ⟨10.1093/mnras/stz2455⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 489 (4), pp.5530-5546. ⟨10.1093/mnras/stz2455⟩
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
Physics and Astronomy Publications
Monthly Notices of the Royal Astronomical Society, 2019, 489 (4), pp.5530-5546. ⟨10.1093/mnras/stz2455⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2019, 489 (4), pp.5530-5546. ⟨10.1093/mnras/stz2455⟩
Digibug. Repositorio Institucional de la Universidad de Granada
instname
Digital.CSIC. Repositorio Institucional del CSIC
Physics and Astronomy Publications
SIGNALS, the Star formation, Ionized Gas, and Nebular Abundances Legacy Survey, is a large observing programme designed to investigate massive star formation and HII regions in a sample of local extended galaxies. The programme will use the imaging F
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ea4060ea72d95230b1152eb47c10508
https://doi.org/10.1093/mnras/stz2455
https://doi.org/10.1093/mnras/stz2455
Publikováno v:
The Astrophysical Journal. 923:78
We employ ionization-parameter mapping (IPM) to infer the optical depth of HII regions in the northern half of M33. We construct [OIII]$\lambda 5007$/[OII]$\lambda 3727$ and [OIII]$\lambda 5007$/[SII]$\lambda 6724$ ratio maps from narrow-band images
Publikováno v:
Astrophys.J.
Astrophys.J., 2019, 885 (1), pp.15. ⟨10.3847/1538-4357/ab3664⟩
Astrophys.J., 2019, 885 (1), pp.15. ⟨10.3847/1538-4357/ab3664⟩
We present an updated version of POLARIS, a well established code designated for dust polarisation and line radiative transfer (RT) in arbitrary astrophysical environments. We extend the already available capabilities with a synchrotron feature for p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6774012f9091c782597e1f9c2d279fcb
https://hal.archives-ouvertes.fr/hal-02283579
https://hal.archives-ouvertes.fr/hal-02283579
Autor:
Ralf S. Klessen, Simon C. O. Glover, Rodrigo Herrera-Camus, Stefan Reissl, Daniel Rahner, Rüdiger Pakmor, Robert J. J. Grand, Eric W. Pellegrini
Publikováno v:
MNRAS
We present a novel method to model galactic scale star formation and the resulting emission from star clusters and the multi-phase interstellar medium. We combine global parameters, such as SFR and CMF, with {\sc warpfield} which provides a descripti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::366b72089ee485ac8719628ad44d6a96
http://arxiv.org/abs/1905.04158
http://arxiv.org/abs/1905.04158