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imfABC.bib
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imfABC.bib
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%% This BibTeX bibliography file was created using BibDesk.
%% http://bibdesk.sourceforge.net/
%% Created for jc3222 at 2018-07-05 13:50:49 -0400
%% Saved with string encoding Unicode (UTF-8)
@article{Bate2014,
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Date-Added = {2018-07-05 17:50:40 +0000},
Date-Modified = {2018-07-05 17:50:49 +0000},
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Publisher = {Oxford University Press},
Title = {The statistical properties of stars and their dependence on metallicity: the effects of opacity},
Volume = {442},
Year = {2014}}
@article{Pokhrel:2018nr,
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Date-Added = {2018-06-28 14:06:21 +0000},
Date-Modified = {2018-06-28 14:06:21 +0000},
Journal = {The Astrophysical Journal},
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Publisher = {IOP Publishing},
Title = {Hierarchical fragmentation in the Perseus molecular cloud: From the cloud scale to protostellar objects},
Volume = {853},
Year = {2018}}
@article{Dokkum:2010fk,
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Date-Added = {2018-06-19 20:10:26 +0000},
Date-Modified = {2018-06-19 20:10:26 +0000},
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Year = {2010}}
@article{Chabrier:2003om,
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Date-Added = {2018-06-14 13:58:54 +0000},
Date-Modified = {2018-06-19 20:28:21 +0000},
Journal = {The Astrophysical Journal Letters},
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Publisher = {IOP Publishing},
Title = {{The galactic disk mass function: reconciliation of the Hubble space telescope and nearby determinations}},
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Year = {2003}}
@article{Chabrier:2003oq,
Author = {Chabrier, Gilles},
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Date-Modified = {2018-06-14 13:56:43 +0000},
Journal = {Publications of the Astronomical Society of the Pacific},
Number = {809},
Pages = {763},
Publisher = {IOP Publishing},
Title = {Galactic stellar and substellar initial mass function},
Volume = {115},
Year = {2003}}
@book{IMF50,
Date-Added = {2018-06-14 12:23:48 +0000},
Date-Modified = {2018-06-14 12:26:34 +0000},
Editor = {Edvidge Corebelli and Francesco Palla and Hans Zinnecker},
Publisher = {Springer},
Series = {Astrophysics and Space Science Library},
Title = {The initial mass function 50 years later},
Volume = {327},
Year = {2005}}
@article{Weisz:2015kx,
Author = {Weisz, Daniel R and Johnson, L Clifton and Foreman-Mackey, Daniel and Dolphin, Andrew E and Beerman, Lori C and Williams, Benjamin F and Dalcanton, Julianne J and Rix, Hans-Walter and Hogg, David W and Fouesneau, Morgan and others},
Date-Added = {2018-06-14 11:10:09 +0000},
Date-Modified = {2018-06-19 20:33:14 +0000},
Journal = {The Astrophysical Journal},
Number = {2},
Pages = {198},
Publisher = {IOP Publishing},
Title = {{The High-Mass Stellar Initial Mass Function in M31 Clusters}},
Volume = {806},
Year = {2015}}
@article{Da-Rio:2010aa,
Author = {Da Rio, Nicola and Robberto, Massimo and Soderblom, David R and Panagia, Nino and Hillenbrand, Lynne A and Palla, Francesco and Stassun, Keivan G},
Date-Added = {2018-05-29 13:13:09 +0000},
Date-Modified = {2018-06-19 20:28:51 +0000},
Journal = {The Astrophysical Journal},
Number = {2},
Pages = {1092},
Publisher = {IOP Publishing},
Title = {{A multi-color optical survey of the Orion Nebula cluster. II. The HR diagram}},
Volume = {722},
Year = {2010}}
@book{Chaisson:2011,
Author = {Chaisson, Eric and McMillan, Stephen},
Date-Added = {2018-02-20 14:58:36 +0000},
Date-Modified = {2018-02-20 15:08:41 +0000},
Edition = {7th},
Publisher = {Addison-Wesley},
Title = {Astronomy today},
Year = {2011}}
@article{McMillan:2016uq,
Author = {McMillan, Paul J},
Date-Added = {2018-02-19 16:21:24 +0000},
Date-Modified = {2018-06-19 20:31:31 +0000},
Journal = {Monthly Notices of the Royal Astronomical Society},
Pages = {stw2759},
Publisher = {Oxford University Press},
Title = {{The mass distribution and gravitational potential of the Milky Way}},
Year = {2016}}
@article{McMillan:2011fk,
Author = {McMillan, Paul J},
Date-Added = {2018-02-19 16:12:15 +0000},
Date-Modified = {2018-06-19 20:31:24 +0000},
Journal = {Monthly Notices of the Royal Astronomical Society},
Number = {3},
Pages = {2446--2457},
Publisher = {Blackwell Publishing Ltd Oxford, UK},
Title = {{Mass models of the Milky Way}},
Volume = {414},
Year = {2011}}
@article{Geha2013,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...771...29G},
Archiveprefix = {arXiv},
Author = {{Geha}, M. and {Brown}, T.~M. and {Tumlinson}, J. and {Kalirai}, J.~S. and {Simon}, J.~D. and {Kirby}, E.~N. and {VandenBerg}, D.~A. and {Mu{\~n}oz}, R.~R. and {Avila}, R.~J. and {Guhathakurta}, P. and {Ferguson}, H.~C.},
Doi = {10.1088/0004-637X/771/1/29},
Eid = {29},
Eprint = {1304.7769},
Journal = {The Astrophysical Journal},
Keywords = {galaxies: dwarf, galaxies: evolution, galaxies: photometry, galaxies: stellar content, Local Group},
Month = jul,
Pages = {29},
Title = {{The Stellar Initial Mass Function of Ultra-faint Dwarf Galaxies: Evidence for IMF Variations with Galactic Environment}},
Volume = 771,
Year = 2013,
Bdsk-Url-1 = {http://dx.doi.org/10.1088/0004-637X/771/1/29}}
@article{Dib2017,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2017MNRAS.464.1738D},
Archiveprefix = {arXiv},
Author = {{Dib}, S. and {Schmeja}, S. and {Hony}, S.},
Doi = {10.1093/mnras/stw2465},
Eprint = {1605.08438},
Journal = {Monthly Notices of the Royal Astronomical Society},
Keywords = {stars: luminosity function, mass function, stars: massive, stars: statistics, open clusters and associations: general, Galaxy: stellar content},
Month = jan,
Pages = {1738-1752},
Title = {{Massive stars reveal variations of the stellar initial mass function in the Milky Way stellar clusters}},
Volume = 464,
Year = 2017,
Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stw2465}}
@article{Dib2014,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2014MNRAS.444.1957D},
Archiveprefix = {arXiv},
Author = {{Dib}, S.},
Doi = {10.1093/mnras/stu1521},
Eprint = {1405.3287},
Journal = {Monthly Notices of the Royal Astronomical Society},
Keywords = {stars: formation, stars: luminosity function, mass function, stars: statistics, open clusters and associations: general, galaxies: clusters: general},
Month = oct,
Pages = {1957-1981},
Title = {{Testing the universality of the IMF with Bayesian statistics: young clusters}},
Volume = 444,
Year = 2014,
Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stu1521}}
@article{Jose2017,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2017ApJ...836...98J},
Archiveprefix = {arXiv},
Author = {{Jose}, J. and {Herczeg}, G.~J. and {Samal}, M.~R. and {Fang}, Q. and {Panwar}, N.},
Doi = {10.3847/1538-4357/836/1/98},
Eid = {98},
Eprint = {1612.00697},
Journal = {The Astrophysical Journal},
Keywords = {stars: formation, stars: luminosity function, mass function},
Month = feb,
Pages = {98},
Primaryclass = {astro-ph.SR},
Title = {{The Low-mass Population in the Young Cluster Stock 8: Stellar Properties and Initial Mass Function}},
Volume = 836,
Year = 2017,
Bdsk-Url-1 = {http://dx.doi.org/10.3847/1538-4357/836/1/98}}
@article{Ashworth2017,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2017MNRAS.469.2464A},
Archiveprefix = {arXiv},
Author = {{Ashworth}, G. and {Fumagalli}, M. and {Krumholz}, M.~R. and {Adamo}, A. and {Calzetti}, D. and {Chandar}, R. and {Cignoni}, M. and {Dale}, D. and {Elmegreen}, B.~G. and {Gallagher}, III, J.~S. and {Gouliermis}, D.~A. and {Grasha}, K. and {Grebel}, E.~K. and {Johnson}, K.~E. and {Lee}, J. and {Tosi}, M. and {Wofford}, A.},
Doi = {10.1093/mnras/stx935},
Eprint = {1705.02980},
Journal = {Monthly Notices of the Royal Astronomical Society},
Keywords = {methods: statistical, stars: luminosity function, mass function, galaxies: individual: NGC 628, galaxies: star clusters: general},
Month = aug,
Pages = {2464-2480},
Title = {{Exploring the IMF of star clusters: a joint SLUG and LEGUS effort}},
Volume = 469,
Year = 2017,
Bdsk-Url-1 = {http://dx.doi.org/10.1093/mnras/stx935}}
@article{Kalari2018,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2018arXiv180101490K},
Archiveprefix = {arXiv},
Author = {{Kalari}, V.~M. and {Carraro}, G. and {Evans}, C.~J. and {Rubio}, M.},
Eprint = {1801.01490},
Journal = {ArXiv e-prints},
Keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
Month = jan,
Primaryclass = {astro-ph.SR},
Title = {{The Magellanic Bridge cluster NGC 796: Deep optical AO imaging reveals the stellar content and initial mass function of a massive open cluster}},
Year = 2018}
@inproceedings{Woosley2015,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2015ASSL..412..199W},
Archiveprefix = {arXiv},
Author = {{Woosley}, S.~E. and {Heger}, A.},
Booktitle = {Very Massive Stars in the Local Universe},
Doi = {10.1007/978-3-319-09596-7_7},
Editor = {{Vink}, J.~S.},
Eprint = {1406.5657},
Keywords = {Physics},
Pages = {199},
Primaryclass = {astro-ph.SR},
Series = {Astrophysics and Space Science Library},
Title = {{The Deaths of Very Massive Stars}},
Volume = 412,
Year = 2015,
Bdsk-Url-1 = {http://dx.doi.org/10.1007/978-3-319-09596-7_7}}
@article{Li2017,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2017ApJ...834...69L},
Archiveprefix = {arXiv},
Author = {{Li}, H. and {Gnedin}, O.~Y. and {Gnedin}, N.~Y. and {Meng}, X. and {Semenov}, V.~A. and {Kravtsov}, A.~V.},
Doi = {10.3847/1538-4357/834/1/69},
Eid = {69},
Eprint = {1608.03244},
Journal = {The Astrophysical Journal},
Keywords = {cosmology: theory, galaxies: formation, galaxies: star clusters: general},
Month = jan,
Pages = {69},
Title = {{Star Cluster Formation in Cosmological Simulations. I. Properties of Young Clusters}},
Volume = 834,
Year = 2017,
Bdsk-Url-1 = {http://dx.doi.org/10.3847/1538-4357/834/1/69}}
@article{Beccari2017,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2017A%26A...604A..22B},
Archiveprefix = {arXiv},
Author = {{Beccari}, G. and {Petr-Gotzens}, M.~G. and {Boffin}, H.~M.~J. and {Romaniello}, M. and {Fedele}, D. and {Carraro}, G. and {De Marchi}, G. and {de Wit}, W.-J. and {Drew}, J.~E. and {Kalari}, V.~M. and {Manara}, C.~F. and {Martin}, E.~L. and {Mieske}, S. and {Panagia}, N. and {Testi}, L. and {Vink}, J.~S. and {Walsh}, J.~R. and {Wright}, N.~J.},
Doi = {10.1051/0004-6361/201730432},
Eid = {A22},
Eprint = {1705.09496},
Journal = {Astronomy \& Astrophysics},
Keywords = {stars: pre-main sequence, open clusters and associations: individual: Orion},
Month = jul,
Pages = {A22},
Primaryclass = {astro-ph.SR},
Title = {{A tale of three cities. OmegaCAM discovers multiple sequences in the color-magnitude diagram of the Orion Nebula Cluster}},
Volume = 604,
Year = 2017,
Bdsk-Url-1 = {http://dx.doi.org/10.1051/0004-6361/201730432}}
@article{Hillenbrand1998,
Abstract = {We use optical and near-infrared star counts to explore the structure and dynamics of the Orion Nebula Cluster (ONC). This very young (<1 Myr) cluster is not circularly symmetric in projection but is elongated north-south in a manner similar to the molecular gas distribution in the region, suggesting that the stellar system may still reflect the geometry of the protocluster cloud. Azimuthally averaged stellar source counts compare well with simple spherically symmetric, single-mass King cluster models. The model fits suggest that the inner Trapezium region should be regarded as the core of the ONC, not as a distinct entity as sometimes advocated. We estimate that the core radius of the cluster is 0.16-0.21 pc and that the central stellar density approaches 2 × 10 4 stars pc -3 . Adopting the stellar velocity dispersion from published proper-motion studies, virial equilibrium would require a total mass within about 2 pc of the Trapezium of ~4500 M ☉ , slightly more than twice the mass of the known stellar population and comparable to the estimated mass in molecular gas projected onto the same region of the sky. If ##IMG## [http://ej.iop.org/icons/Entities/gtrsim.gif] {gtrsim} 20% of the remaining molecular gas is converted into stars, thus adding to the binding mass, given that the present stellar population alone has a total energy close to zero, the ONC is likely to produce a gravitationally bound cluster. The ONC also exhibits mass segregation, with the most massive (Trapezium) stars clearly concentrated toward the center of the cluster and some evidence for the degree of central concentration to decrease with decreasing mass down to 1-2 M ☉ , as would be expected for general mass segregation. Given the extreme youth of the stars compared with the estimated range of collisional relaxation times, the mass segregation is unlikely to be the result of cluster relaxation. Instead, we suggest that the mass segregation reflects a preference for higher mass stars to form in dense, central cluster regions.},
Author = {Lynne A. Hillenbrand and Lee W. Hartmann},
Journal = {The Astrophysical Journal},
Number = {2},
Pages = {540},
Title = {A Preliminary Study of the Orion Nebula Cluster Structure and Dynamics},
Url = {http://stacks.iop.org/0004-637X/492/i=2/a=540},
Volume = {492},
Year = {1998},
Bdsk-Url-1 = {http://stacks.iop.org/0004-637X/492/i=2/a=540}}
@article{Lin2015,
Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
Adsurl = {http://adsabs.harvard.edu/abs/2015A%26A...583A..70L},
Archiveprefix = {arXiv},
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