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Early Star Formation Traced by Water Masers. / Ladeyschikov, Dmitry.
в: Proceedings of the International Astronomical Union, Том 18, № S380, 01.12.2022, стр. 230-231.

Результаты исследований: Вклад в журналМатериалы конференцииРецензирование

Harvard

Ladeyschikov, D 2022, 'Early Star Formation Traced by Water Masers', Proceedings of the International Astronomical Union, Том. 18, № S380, стр. 230-231. https://doi.org/10.1017/S1743921323003290

APA

Ladeyschikov, D. (2022). Early Star Formation Traced by Water Masers. Proceedings of the International Astronomical Union, 18(S380), 230-231. https://doi.org/10.1017/S1743921323003290

Vancouver

Ladeyschikov D. Early Star Formation Traced by Water Masers. Proceedings of the International Astronomical Union. 2022 дек. 1;18(S380):230-231. doi: 10.1017/S1743921323003290

Author

Ladeyschikov, Dmitry. / Early Star Formation Traced by Water Masers. в: Proceedings of the International Astronomical Union. 2022 ; Том 18, № S380. стр. 230-231.

BibTeX

@article{64d3060cc42a470ba559797ec1c570ce,
title = "Early Star Formation Traced by Water Masers",
abstract = "In this study, the correlation between 22 GHz water masers and other maser species with far infrared/submillimeter (FIR/sub-mm) sources is investigated. Comparing luminosity to mass ratio (L/M) of FIR/sub-mm clumps linked to different maser species, 22 GHz water masers have significantly lower L/M values than 6.7 GHz methanol and 1665 MHz OH masers. This suggests 22 GHz water masers may precede them in the evolution timeline of SFRs. The close association between water masers and FIR/sub-mm sources provides insight into maser pumping conditions and evolutionary stages.",
author = "Dmitry Ladeyschikov",
year = "2022",
month = dec,
day = "1",
doi = "10.1017/S1743921323003290",
language = "English",
volume = "18",
pages = "230--231",
journal = "Proceedings of the International Astronomical Union",
issn = "1743-9213",
publisher = "Cambridge University Press",
number = "S380",

}

RIS

TY - JOUR

T1 - Early Star Formation Traced by Water Masers

AU - Ladeyschikov, Dmitry

PY - 2022/12/1

Y1 - 2022/12/1

N2 - In this study, the correlation between 22 GHz water masers and other maser species with far infrared/submillimeter (FIR/sub-mm) sources is investigated. Comparing luminosity to mass ratio (L/M) of FIR/sub-mm clumps linked to different maser species, 22 GHz water masers have significantly lower L/M values than 6.7 GHz methanol and 1665 MHz OH masers. This suggests 22 GHz water masers may precede them in the evolution timeline of SFRs. The close association between water masers and FIR/sub-mm sources provides insight into maser pumping conditions and evolutionary stages.

AB - In this study, the correlation between 22 GHz water masers and other maser species with far infrared/submillimeter (FIR/sub-mm) sources is investigated. Comparing luminosity to mass ratio (L/M) of FIR/sub-mm clumps linked to different maser species, 22 GHz water masers have significantly lower L/M values than 6.7 GHz methanol and 1665 MHz OH masers. This suggests 22 GHz water masers may precede them in the evolution timeline of SFRs. The close association between water masers and FIR/sub-mm sources provides insight into maser pumping conditions and evolutionary stages.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85185815250

U2 - 10.1017/S1743921323003290

DO - 10.1017/S1743921323003290

M3 - Conference article

VL - 18

SP - 230

EP - 231

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S380

ER -

ID: 53846665