Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Alexander P. S. Hygate"'
Autor:
Hanae Inami, Hiddo S B Algera, Sander Schouws, Laura Sommovigo, Rychard Bouwens, Renske Smit, Mauro Stefanon, Rebecca A A Bowler, Ryan Endsley, Andrea Ferrara, Pascal Oesch, Daniel Stark, Manuel Aravena, Laia Barrufet, Elisabete da Cunha, Pratika Dayal, Ilse De Looze, Yoshinobu Fudamoto, Valentino Gonzalez, Luca Graziani, Jacqueline A Hodge, Alexander P S Hygate, Themiya Nanayakkara, Andrea Pallottini, Dominik A Riechers, Raffaella Schneider, Michael Topping, Paul van der Werf
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Inami, H, Algera, H S B, Schouws, S, Sommovigo, L, Bouwens, R, Smit, R, Stefanon, M, Bowler, R A A, Endsley, R, Ferrara, A, Oesch, P, Stark, D, Aravena, M, Barrufet, L, da Cunha, E, Dayal, P, De Looze, I, Fudamoto, Y, Gonzalez, V, Graziani, L, Hodge, J A, Hygate, A P S, Nanayakkara, T, Pallottini, A, Riechers, D A, Schneider, R, Topping, M & van der Werf, P 2022, ' The ALMA REBELS Survey : dust continuum detections at z > 6.5 ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 3, pp. 3126-3143 . https://doi.org/10.1093/mnras/stac1779
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 515(3), 3126-3143
Monthly Notices of the Royal Astronomical Society, 515, 3126-3143. Oxford University Press
Inami, H, Algera, H S B, Schouws, S, Sommovigo, L, Bouwens, R, Smit, R, Stefanon, M, Bowler, R A A, Endsley, R, Ferrara, A, Oesch, P, Stark, D, Aravena, M, Barrufet, L, da Cunha, E, Dayal, P, De Looze, I, Fudamoto, Y, Gonzalez, V, Graziani, L, Hodge, J A, Hygate, A P S, Nanayakkara, T, Pallottini, A, Riechers, D A, Schneider, R, Topping, M & van der Werf, P 2022, ' The ALMA REBELS Survey : dust continuum detections at z > 6.5 ', Monthly Notices of the Royal Astronomical Society, vol. 515, no. 3, pp. 3126-3143 . https://doi.org/10.1093/mnras/stac1779
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society, 515(3), 3126-3143
Monthly Notices of the Royal Astronomical Society, 515, 3126-3143. Oxford University Press
We report 18 dust continuum detections ($\geq 3.3\sigma$) at $\sim88{\rm \mu m}$ and $158{\rm \mu m}$ out of 49 ultraviolet(UV)-bright galaxies ($M_{\rm UV} < -21.3$ mag) at $z>6.5$, observed by the Cycle-7 ALMA Large Program, REBELS and its pilot pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56edd121428e99c5ef53aaab07f0b6a0
Autor:
Hiddo S B Algera, Hanae Inami, Pascal A Oesch, Laura Sommovigo, Rychard J Bouwens, Michael W Topping, Sander Schouws, Mauro Stefanon, Daniel P Stark, Manuel Aravena, Laia Barrufet, Elisabete da Cunha, Pratika Dayal, Ryan Endsley, Andrea Ferrara, Yoshinobu Fudamoto, Valentino Gonzalez, Luca Graziani, Jacqueline A Hodge, Alexander P S Hygate, Ilse de Looze, Themiya Nanayakkara, Raffaella Schneider, Paul P van der Werf
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 518(4), 6142-6157. Oxford University Press
Algera, H S B, Inami, H, Oesch, P A, Sommovigo, L, Bouwens, R J, Topping, M W, Schouws, S, Stefanon, M, Stark, D P, Aravena, M, Barrufet, L, da Cunha, E, Dayal, P, Endsley, R, Ferrara, A, Fudamoto, Y, Gonzalez, V, Graziani, L, Hodge, J A, Hygate, A P S, de Looze, I, Nanayakkara, T, Schneider, R & van der Werf, P P 2023, ' The ALMA REBELS survey : the dust-obscured cosmic star formation rate density at redshift 7 ', Monthly Notices of the Royal Astronomical Society, vol. 518, no. 4, pp. 6142-6157 . https://doi.org/10.1093/mnras/stac3195
Algera, H S B, Inami, H, Oesch, P A, Sommovigo, L, Bouwens, R J, Topping, M W, Schouws, S, Stefanon, M, Stark, D P, Aravena, M, Barrufet, L, da Cunha, E, Dayal, P, Endsley, R, Ferrara, A, Fudamoto, Y, Gonzalez, V, Graziani, L, Hodge, J A, Hygate, A P S, de Looze, I, Nanayakkara, T, Schneider, R & van der Werf, P P 2023, ' The ALMA REBELS survey : the dust-obscured cosmic star formation rate density at redshift 7 ', Monthly Notices of the Royal Astronomical Society, vol. 518, no. 4, pp. 6142-6157 . https://doi.org/10.1093/mnras/stac3195
Cosmic dust is an essential component shaping both the evolution of galaxies and their observational signatures. How quickly dust builds up in the early Universe remains an open question that requires deep observations at (sub-)millimeter wavelengths
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::69970da32f4cc03e6244baa80843bef5
https://doi.org/10.48550/arxiv.2208.08243
https://doi.org/10.48550/arxiv.2208.08243
Autor:
Alexander P. S. Hygate, A. F. McLeod, Steven N. Longmore, Mélanie Chevance, Daniel T. Haydon, Linda J. Tacconi, Ewine F. van Dishoeck, J. M. Diederik Kruijssen, Andreas Schruba, Julianne J. Dalcanton
Publikováno v:
Nature
The physics of star formation and the deposition of mass, momentum, and energy into the interstellar medium by massive stars (`feedback') are the main uncertainties in modern cosmological simulations of galaxy formation and evolution. These processes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be9a4e942baea348e2ef21aa95ec2989
http://europepmc.org/articles/PMC6544524
http://europepmc.org/articles/PMC6544524
Autor:
Alexander P. S. Hygate, Cinthya N. Herrera, Dyas Utomo, Mélanie Chevance, Kathryn Kreckel, Antonio Usero, Jiayi Sun, Ismael Pessa, Daniel A. Dale, Simon C. O. Glover, Andreas Schruba, Sharon E. Meidt, Jérôme Pety, Kathryn Grasha, Diane Cormier, Adam K. Leroy, Toshiki Saito, Frank Bigiel, Annie Hughes, Miguel Querejeta, Eva Schinnerer, Philipp Lang, Guillermo A. Blanc, Erik Rosolowsky, J. M. Diederik Kruijssen, Christopher Faesi, María J. Jiménez-Donaire, Kazimierz Sliwa
Publikováno v:
ASTRONOMY & ASTROPHYSICS
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 634, pp.A121. ⟨10.1051/0004-6361/201936060⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 634, pp.A121. ⟨10.1051/0004-6361/201936060⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 634, pp.A121. ⟨10.1051/0004-6361/201936060⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 634, pp.A121. ⟨10.1051/0004-6361/201936060⟩
Cloud-scale surveys of molecular gas reveal the link between molecular clouds properties and star formation (SF) across a range of galactic environments. Cloud populations in galaxy disks are considered to be representative of the `normal' SF. At hig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ca3ec0252b7275e7277c079b926ffaa0
https://biblio.ugent.be/publication/8747437/file/01GKKK5B60D152MVG59M0HVWS3
https://biblio.ugent.be/publication/8747437/file/01GKKK5B60D152MVG59M0HVWS3
Autor:
Janice C. Lee, Philipp Lang, Cinthya N. Herrera, Christopher M Faesi, Daizhong Liu, Annie Hughes, Jiayi Sun, Guillermo A. Blanc, Frank Bigiel, Alessandro Razza, I-Ting Ho, Brent Groves, A. Usero, J. M. Diederik Kruijssen, Daniel T. Haydon, Steven N. Longmore, Simon C. O. Glover, Mélanie Chevance, Toshiki Saito, Kathryn Kreckel, Jérôme Pety, Jonathan D. Henshaw, Dyas Utomo, Eric Emsellem, Alexander P. S. Hygate, Adam K. Leroy, Sarah M R Jeffreson, Eva Schinnerer, Miguel Querejeta, Sharon Meidt, Andreas Schruba, Erik Rosolowsky
Publikováno v:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 493, pp.2872-2909. ⟨10.1093/mnras/stz3525⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2020, 493, pp.2872-2909. ⟨10.1093/mnras/stz3525⟩
It remains a major challenge to derive a theory of cloud-scale ($\lesssim100$ pc) star formation and feedback, describing how galaxies convert gas into stars as a function of the galactic environment. Progress has been hampered by a lack of robust em
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2145022efaf1bf41f21ef3a324cc94b0
http://arxiv.org/abs/1911.03479
http://arxiv.org/abs/1911.03479
Autor:
J. Pety, Eric J. Murphy, Andreas Schruba, Christopher M Faesi, S. C. O. Glover, Dyas Utomo, Sharon E. Meidt, Santiago García-Burillo, Eva Schinnerer, M. Chevance, Adam K. Leroy, Emmanuel Momjian, J. M. D. Kruijssen, Frank Bigiel, Alexander P. S. Hygate, M. Gallagher, A. Usero, Miguel Querejeta, M. J. Jimenez-Donaire, Erik Rosolowsky
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A19. ⟨10.1051/0004-6361/201834915⟩
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A19. ⟨10.1051/0004-6361/201834915⟩
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics
It remains unclear what sets the efficiency with which molecular gas transforms into stars. Here we present a new VLA map of the spiral galaxy M51 in 33GHz radio continuum, an extinction-free tracer of star formation, at 3" scales (~100pc). We combin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7332237ddab7012f0d4e44c277a71683
https://hal.archives-ouvertes.fr/hal-03081719
https://hal.archives-ouvertes.fr/hal-03081719
Autor:
Daniel T. Haydon, Mark R. Krumholz, Andreas Schruba, Alexander P. S. Hygate, J. M. Diederik Kruijssen, Steven N. Longmore, Mélanie Chevance
We recently presented a new statistical method to constrain the physics of star formation and feedback on the cloud scale by reconstructing the underlying evolutionary timeline. However, by itself this new method only recovers the relative durations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::837614b0d8be389aca7a19fa955cb8d4
http://arxiv.org/abs/1810.10897
http://arxiv.org/abs/1810.10897
Autor:
Brent Groves, Frank Bigiel, Annie Hughes, Erik Rosolowsky, J. M. Diederik Kruijssen, Alberto D. Bolatto, Alexander P. S. Hygate, Miguel Querejeta, Antonio Usero, Guillermo A. Blanc, Andreas Schruba, Cinthya N. Herrera, Jiayi Sun, Sharon E. Meidt, Jérôme Pety, Mélanie Chevance, Dyas Utomo, Adam K. Leroy, Eva Schinnerer
Publikováno v:
The Astrophysical Journal
ASTROPHYSICAL JOURNAL
ASTROPHYSICAL JOURNAL
We measure the velocity dispersion, $\sigma$, and surface density, $\Sigma$, of the molecular gas in nearby galaxies from CO spectral line cubes with spatial resolution $45$-$120$ pc, matched to the size of individual giant molecular clouds. Combinin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3932235b28bb3b7744f13fcd81ce959c
http://arxiv.org/abs/1805.00937
http://arxiv.org/abs/1805.00937
Autor:
Alexander P. S. Hygate, Chia-Yu Hu, Andreas Schruba, J. M. Diederik Kruijssen, Daniel T. Haydon, Steven N. Longmore
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The cloud-scale physics of star formation and feedback represent the main uncertainty in galaxy formation studies. Progress is hampered by the limited empirical constraints outside the restricted environment of the Local Group. In particular, the poo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5c0cdb63dee932cb1d35c71c24a927b
Autor:
Jiayi Sun, Antonio Usero, Kathryn Kreckel, Mélanie Chevance, Miguel Querejeta, Dyas Utomo, Adam K. Leroy, Guillermo A. Blanc, Eve C. Ostriker, Andreas Schruba, Erik Rosolowsky, Frank Bigiel, Karin Sandstrom, Cinthya N. Herrera, Alexander P. S. Hygate, Jérôme Pety, Eva Schinnerer, J. M. Diederik Kruijssen, Eric Emsellem
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical journal letters, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical Journal
The Astrophysical journal letters, Bristol : IOP Publishing, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical journal letters, 2018, 861 (2), pp.L18. ⟨10.3847/2041-8213/aacf8f⟩
The Astrophysical Journal
We estimate the star formation efficiency per gravitational free fall time, $\epsilon_{\rm ff}$, from observations of nearby galaxies with resolution matched to the typical size of a Giant Molecular Cloud. This quantity, $\epsilon_{\rm ff}$, is theor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bacc5f0d636d45828fe834899476b93