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Astrophysical #Journal Letters	2041-8205

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Ord.	Autor	Género	Institución - País
1	Zhang, Yichen	-	RIKEN - Japón RIKEN Cluster for Pioneering Research - Japón
2	TANAKA, KEI E., I	Mujer	Osaka Univ - Japón Natl Astron Observ Japan - Japón Osaka University - Japón National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón
3	Rosero, Viviana	Mujer	Natl Radio Astron Observ - Estados Unidos National Radio Astronomy Observatory Socorro - Estados Unidos
4	Tan, Jonathan C.	Hombre	Chalmers Univ Technol - Suecia UNIV VIRGINIA - Estados Unidos Chalmers University of Technology - Suecia University of Virginia - Estados Unidos
5	Marvil, Joshua	Hombre	Natl Radio Astron Observ - Estados Unidos National Radio Astronomy Observatory Socorro - Estados Unidos
6	Cheng, Yu	-	UNIV VIRGINIA - Estados Unidos University of Virginia - Estados Unidos
7	Liu, Mengyao	-	UNIV VIRGINIA - Estados Unidos University of Virginia - Estados Unidos
8	Beltran, Maria T.	Mujer	Osserv Astrofis Arcetri - Italia Osservatorio Astrofisico Di Arcetri - Italia
9	GARAY BRIGNARDELLO, GUIDO ALEJANDRO	Hombre	Universidad de Chile - Chile

Ord.

Autor

Género

Institución - País

Zhang, Yichen

RIKEN - Japón
RIKEN Cluster for Pioneering Research - Japón

TANAKA, KEI E., I

Mujer

Osaka Univ - Japón
Natl Astron Observ Japan - Japón
Osaka University - Japón
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón

Rosero, Viviana

Mujer

Natl Radio Astron Observ - Estados Unidos
National Radio Astronomy Observatory Socorro - Estados Unidos

Tan, Jonathan C.

Hombre

Chalmers Univ Technol - Suecia
UNIV VIRGINIA - Estados Unidos
Chalmers University of Technology - Suecia
University of Virginia - Estados Unidos

Marvil, Joshua

Hombre

Natl Radio Astron Observ - Estados Unidos
National Radio Astronomy Observatory Socorro - Estados Unidos

Cheng, Yu

UNIV VIRGINIA - Estados Unidos
University of Virginia - Estados Unidos

Liu, Mengyao

UNIV VIRGINIA - Estados Unidos
University of Virginia - Estados Unidos

Beltran, Maria T.

Mujer

Osserv Astrofis Arcetri - Italia
Osservatorio Astrofisico Di Arcetri - Italia

GARAY BRIGNARDELLO, GUIDO ALEJANDRO

Hombre

Universidad de Chile - Chile

Fuente
University of Virginia
JSPS KAKENHI grant
CONICYT project
NAOJ ALMA Scientific Research grant
ERC project MSTAR
RIKEN Special Postdoctoral Researcher Program
Alberta Livestock and Meat Agency
National Radio Astronomy Observatory
Horizon 2020 Framework Programme
Istituto Nazionale di Astrofisica
Osaka University
Universidad de Chile, Casilla 36-D
Chalmers Tekniska Högskola
Japan Department of Earth and Space Science
RIKEN Cluster for Pioneering Research

Fuente

University of Virginia

JSPS KAKENHI grant

CONICYT project

NAOJ ALMA Scientific Research grant

ERC project MSTAR

RIKEN Special Postdoctoral Researcher Program

Alberta Livestock and Meat Agency

National Radio Astronomy Observatory

Horizon 2020 Framework Programme

Istituto Nazionale di Astrofisica

Osaka University

Universidad de Chile, Casilla 36-D

Chalmers Tekniska Högskola

Japan Department of Earth and Space Science

RIKEN Cluster for Pioneering Research

Agradecimiento
We thank Boy Lankhaar for valuable discussions. This Letter makes use of the following ALMA data: ADS/JAO. ALMA#2015.1.01454.S, and ADS/JAO. ALMA#2017.1. 00181.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. Y.Z. acknowledges supports from RIKEN Special Postdoctoral Researcher Program and JSPS KAKENHI grant JP19K14774. K.E.I.T. acknowledges support from NAOJ ALMA Scientific Research grant No. 2017-05A, JSPS KAKENHI grant Nos. JP19H05080, JP19K14760. J.C.T. acknowledges support from ERC project MSTAR. G.G. acknowledges support from CONICYT project AFB-170002.
Yichen Zhang Kei E. I. Tanaka Viviana Rosero Jonathan C. Tan Joshua Marvil Yu Cheng Mengyao Liu Maria T. Beltr�n Guido Garay Yichen Zhang Kei E. I. Tanaka Viviana Rosero Jonathan C. Tan Joshua Marvil Yu Cheng Mengyao Liu Maria T. Beltr�n Guido Garay Star and Planet Formation Laboratory, RIKEN Cluster for Pioneering Research, Wako, Saitama 351-0198, Japan Department of Earth and Space Science, Osaka University, Toyonaka, Osaka 560-0043, Japan ALMA Project, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, NM 87801, USA Department of Space, Earth & Environment, Chalmers University of Technology, SE-412 96 Gothenburg, Sweden Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USA INAF—Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy Departamento de Astronom�a, Universidad de Chile, Casilla 36-D, Santiago, Chile Yichen Zhang, Kei E. I. Tanaka, Viviana Rosero, Jonathan C. Tan, Joshua Marvil, Yu Cheng, Mengyao Liu, Maria T. Beltr�n and Guido Garay 2019-11-20 2019-11-13 13:25:36 cgi/release: Article released bin/incoming: New from .zip Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence . Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. JSPS KAKENHI JP19K14774 JSPS KAKENHI JP19H05080 JSPS KAKENHI JP19K14760 ERC MSTAR CONICYT AFB-170002 yes Massive protostars generate strong radiation feedback, which may help set the mass that they achieve by the end of the accretion process. Studying such feedback is therefore crucial for understanding the formation of massive stars. We report the discovery of a photoionized bipolar outflow toward the massive protostar G45.47+0.05 using high-resolution observations at 1.3 mm with the Atacama Large Millimeter/Submillimeter Array (ALMA) and at 7 mm with the Karl G. Jansky Very Large Array (VLA). By modeling the free–free continuum, the ionized outflow is found to be a photoevaporation flow with an electron temperature of 10,000 K and an electron number density of ∼1.5�נ10 7 cm −3 at the center, launched from a disk of radius of 110 au. H30 α hydrogen recombination line emission shows strong maser amplification, with G45 being one of very few sources to show such millimeter recombination line masers. The mass of the driving source is estimated to be 30–50 M ⊙ based on the derived ionizing photon rate, or 30–40 M ⊙ based on the H30 α kinematics. The kinematics of the photoevaporated material is dominated by rotation close to the disk plane, while accelerated to outflowing motion above the disk plane. The mass loss rate of the photoevaporation outflow is estimated to be ∼(2–3.5)�נ10 −5 M ⊙ yr −1 . We also found hints of a possible jet embedded inside the wide-angle ionized outflow with nonthermal emissions. The possible coexistence of a jet and a massive photoevaporation outflow suggests that, in spite of the strong photoionization feedback, accretion is still ongoing. � 2019. The American Astronomical Society. Anglada G., Rodríguez L. F. and Carrasco-González C. 2018 A&ARv 26 3 10.1007/s00159-018-0107-z Anglada G., Rodríguez L. F. and Carrasco-González C. A&ARv 0935-4956 26 2018 3 Báez-Rubio A., Martín-Pintado J., Thum C. and Planesas P. 2013 A&A 553 A45 10.1051/0004-6361/201219889 Báez-Rubio A., Martín-Pintado J., Thum C. and Planesas P. A&A 0004-6361 553 2013 A45 Beltrán M. T., Cesaroni R., Moscadelli L. et al 2016 A&A 593 49 10.1051/0004-6361/201628588 Beltrán M. T., Cesaroni R., Moscadelli L. et al A&A 0004-6361 593 2016 49 Briggs D. S. 1995 BAAS 27 1444 Briggs D. S. BAAS 0002-7537 27 1995 1444 Carrasco-González C., Rodríguez L. F., Anglada G. et al 2010 Sci 330 1209 10.1126/science.1195589 Carrasco-González C., Rodríguez L. F., Anglada G. et al Sci 330 2010 1209 Condon J. J. 1997 PASP 109 166 10.1086/133871 Condon J. J. PASP 1538-3873 109 732 166 1997 166 Davies B., Hoare M. G., Lumsden S. L. et al 2011 MNRAS 416 972 10.1111/j.1365-2966.2011.19095.x Davies B., Hoare M. G., Lumsden S. L. et al MNRAS 0035-8711 416 2011 972 De Buizer J. M., Liu M., Tan J. C., Zhang Y. et al 2017 ApJ 843 33 10.3847/1538-4357/aa74c8 De Buizer J. M., Liu M., Tan J. C., Zhang Y. et al ApJ 0004-637X 843 1 33 2017 33 De Buizer J. M., Radomski J. T., Telesco C. M. and Piña R. K. 2005 ApJS 156 179 10.1086/426941 De Buizer J. M., Radomski J. T., Telesco C. M. and Piña R. K. ApJS 0067-0049 156 2 179 2005 179 Draine B. T. 2011 Physics of the Interstellar and Intergalactic Medium (Princeton, NJ: Princeton Univ. Press) 10.1515/9781400839087 Draine B. T. 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Agradecimiento

We thank Boy Lankhaar for valuable discussions. This Letter makes use of the following ALMA data: ADS/JAO. ALMA#2015.1.01454.S, and ADS/JAO. ALMA#2017.1. 00181.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. Y.Z. acknowledges supports from RIKEN Special Postdoctoral Researcher Program and JSPS KAKENHI grant JP19K14774. K.E.I.T. acknowledges support from NAOJ ALMA Scientific Research grant No. 2017-05A, JSPS KAKENHI grant Nos. JP19H05080, JP19K14760. J.C.T. acknowledges support from ERC project MSTAR. G.G. acknowledges support from CONICYT project AFB-170002.

Yichen Zhang Kei E. I. Tanaka Viviana Rosero Jonathan C. Tan Joshua Marvil Yu Cheng Mengyao Liu Maria T. Beltr�n Guido Garay Yichen Zhang Kei E. I. Tanaka Viviana Rosero Jonathan C. Tan Joshua Marvil Yu Cheng Mengyao Liu Maria T. Beltr�n Guido Garay Star and Planet Formation Laboratory, RIKEN Cluster for Pioneering Research, Wako, Saitama 351-0198, Japan Department of Earth and Space Science, Osaka University, Toyonaka, Osaka 560-0043, Japan ALMA Project, National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan National Radio Astronomy Observatory, 1003 Lopezville Road, Socorro, NM 87801, USA Department of Space, Earth & Environment, Chalmers University of Technology, SE-412 96 Gothenburg, Sweden Department of Astronomy, University of Virginia, Charlottesville, VA 22904-4325, USA INAF—Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy Departamento de Astronom�a, Universidad de Chile, Casilla 36-D, Santiago, Chile Yichen Zhang, Kei E. I. Tanaka, Viviana Rosero, Jonathan C. Tan, Joshua Marvil, Yu Cheng, Mengyao Liu, Maria T. Beltr�n and Guido Garay 2019-11-20 2019-11-13 13:25:36 cgi/release: Article released bin/incoming: New from .zip Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence . Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. JSPS KAKENHI JP19K14774 JSPS KAKENHI JP19H05080 JSPS KAKENHI JP19K14760 ERC MSTAR CONICYT AFB-170002 yes Massive protostars generate strong radiation feedback, which may help set the mass that they achieve by the end of the accretion process. Studying such feedback is therefore crucial for understanding the formation of massive stars. We report the discovery of a photoionized bipolar outflow toward the massive protostar G45.47+0.05 using high-resolution observations at 1.3 mm with the Atacama Large Millimeter/Submillimeter Array (ALMA) and at 7 mm with the Karl G. Jansky Very Large Array (VLA). By modeling the free–free continuum, the ionized outflow is found to be a photoevaporation flow with an electron temperature of 10,000 K and an electron number density of ∼1.5�נ10 7 cm −3 at the center, launched from a disk of radius of 110 au. H30 α hydrogen recombination line emission shows strong maser amplification, with G45 being one of very few sources to show such millimeter recombination line masers. The mass of the driving source is estimated to be 30–50 M ⊙ based on the derived ionizing photon rate, or 30–40 M ⊙ based on the H30 α kinematics. The kinematics of the photoevaporated material is dominated by rotation close to the disk plane, while accelerated to outflowing motion above the disk plane. The mass loss rate of the photoevaporation outflow is estimated to be ∼(2–3.5)�נ10 −5 M ⊙ yr −1 . We also found hints of a possible jet embedded inside the wide-angle ionized outflow with nonthermal emissions. The possible coexistence of a jet and a massive photoevaporation outflow suggests that, in spite of the strong photoionization feedback, accretion is still ongoing. � 2019. The American Astronomical Society. Anglada G., Rodríguez L. F. and Carrasco-González C. 2018 A&ARv 26 3 10.1007/s00159-018-0107-z Anglada G., Rodríguez L. F. and Carrasco-González C. A&ARv 0935-4956 26 2018 3 Báez-Rubio A., Martín-Pintado J., Thum C. and Planesas P. 2013 A&A 553 A45 10.1051/0004-6361/201219889 Báez-Rubio A., Martín-Pintado J., Thum C. and Planesas P. A&A 0004-6361 553 2013 A45 Beltrán M. T., Cesaroni R., Moscadelli L. et al 2016 A&A 593 49 10.1051/0004-6361/201628588 Beltrán M. T., Cesaroni R., Moscadelli L. et al A&A 0004-6361 593 2016 49 Briggs D. S. 1995 BAAS 27 1444 Briggs D. S. 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