HI 21 cm observation and mass models of the extremely thin galaxy FGC 1440

Aditya, K.; Kamphuis, P.; Banerjee, A.; Borisov, S.; Mosenkov, A.; Antipova, A.; Makarov, D.

Авторы: Aditya K., Kamphuis Peter, Banerjee Arunima, Borisov Sviatoslav, Mosenkov Aleksandr, Antipova Aleksandra, Makarov Dmitry
Журнал: Monthly Notices of the Royal Astronomical Society
Том: 509
Номер: 3
Год издания: 2022
Издательство: Oxford Journals, Oxford University Press
Местоположение издательства: Oxford, UK, England
Первая страница: 4071
Последняя страница: 4093
DOI: 10.1093/mnras/stab3143
Аннотация: We present observations and models of the kinematics and distribution of neutral hydrogen (HI) in the superthin galaxy FGC 1440 with an optical axial ratio a/b=20.4. Using the Giant Meterwave Radio telescope (GMRT), we imaged the galaxy with a spectral resolution of 1.7 km/s and a spatial resolution of 15"×13.5". We find that FGC 1440 has an asymptotic rotational velocity of 141.8 km/s. The structure of the HI disc in FGC 1440 is that of a typical thin disc warped along the line of sight, but we can not rule out the presence of a central thick HI disc. We find that the dark matter halo in FGC 1440 could be modeled by a pseudo-isothermal (PIS) profile with Rc/Rd<2, where Rc is the core radius of the PIS halo and Rd the exponential stellar disc scale length. We note that in spite of the unusually large axial ratio of FGC 1440, the ratio of the rotational velocity to stellar vertical velocity dispersion, VRot/σz∼5−8, which is comparable to other superthins. Interestingly, unlike previously studied superthin galaxies which are outliers in the log10(j∗)−log10(M∗) relation for ordinary bulgeless disc galaxies, FGC 1440 is found to comply with the same. The values of j for the stars, gas and the baryons in FGC 1440 are consistent with those of normal spiral galaxies with similar mass.
Добавил в систему: Борисов Святослав Борисович

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HI 21 cm observation and mass models of the extremely thin galaxy FGC 1440статья

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