Veronica Amber Allen - Publications

Affiliations: 
2014-2018 Kapteyn Astronomical Institute University of Groningen, Groningen, Netherlands 

6 high-probability publications. We are testing a new system for linking publications to authors. You can help! If you notice any inaccuracies, please sign in and mark papers as correct or incorrect matches. If you identify any major omissions or other inaccuracies in the publication list, please let us know.

Year Citation  Score
2020 Allen V, Tak FFSvd, López-Sepulcre A, Sánchez-Monge Á, Rivilla VM, Cesaroni R. Exploring the formation pathways of formamide near young O-type stars Astronomy and Astrophysics. 636. DOI: 10.1051/0004-6361/201935791  0.344
2018 Maud LT, Cesaroni R, Kumar MSN, Tak FFSvd, Allen V, Hoare MG, Klaassen PD, Harsono D, Hogerheijde MR, Sanchez-Monge A, Schilke P, Ahmadi A, Beltran MT, Beuther H, Csengeri T, et al. Chasing discs around O-type (proto)stars Astronomy and Astrophysics. 620: 31. DOI: 10.15496/Publikation-30958  0.421
2018 Moscadelli L, Rivilla VM, Cesaroni R, Beltrán MT, Sánchez-Monge Á, Schilke P, Mottram JC, Ahmadi A, Allen V, Beuther H, Csengeri T, Etoka S, Galli D, Goddi C, Johnston KG, et al. The feedback of an HC HII region on its parental molecular core Astronomy & Astrophysics. 616: A66. DOI: 10.1051/0004-6361/201832680  0.342
2018 Allen V, Tak FFSvd, Walsh C. Complex cyanides as chemical clocks in hot cores Astronomy and Astrophysics. 616: 67. DOI: 10.1051/0004-6361/201732553  0.344
2017 Cesaroni R, Sánchez-Monge A, Beltrán M~, Johnston KG, Maud LT, Moscadelli L, Mottram J~, Ahmadi A, Allen V, Beuther H, Csengeri T, Etoka S, Fuller GA, Galli D, Galván-Madrid R, et al. Chasing discs around O-type (proto)stars: Evidence from ALMA observations Astronomy and Astrophysics. 602: 1-22. DOI: 10.1051/0004-6361/201630184  0.341
2017 Allen V, Tak FFSvd, Sánchez-Monge Á, Cesaroni R, Beltrán MT. Chemical segregation in hot cores with disk candidates: An investigation with ALMA Astronomy and Astrophysics. 603. DOI: 10.1051/0004-6361/201629118  0.374
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