Double-mode Cepheids from the Zwicky Transient Facility Survey

نویسندگان

چکیده

Multi-mode Cepheids pulsate simultaneously in more than one mode of oscillation. They provide an independent means to test stellar models and pulsation theories. can also be used derive metallicities. In recent years, the number known multi-mode has increased dramatically with discovery a large Galactic double-mode Cepheids. To date, 209 have been detected bulge disk, mostly based on Optical Gravitational Lensing Experiment's (OGLE) catalog. this paper, we conduct comprehensive search for northern sky Zwicky Transient Facility Data Release 5. We found 72 such objects Milky Way. The periods 30 sample already included OGLE catalog show excellent agreement periods. period ratios our new are consistent those Cepheids, as evidenced by their loci so-called `Petersen diagram'. Compared OGLE, completeness Cepheid is around 71\%. much improved temporal sampling offers significant scope find especially at distribution's short-period end.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The galactic double – mode Cepheids

By considering the least–squares fits of the double–mode Cepheid light curves discussed in Paper I we defined their properties by their Fourier parameters and generalized phase differences G i,j. When plotting the latter quantities as a function of the respective order, the second order terms are confined in the region just below 3/2π; the third order terms have π/2 < G i,j < π, the fourth orde...

متن کامل

Study of transient double-mode behaviour of nonlinear models of Cepheids

Nonlinear pulsation models of Cepheids pulsating in first and second overtone modes have been constructed in order to study their transient double-mode behaviour. The purposes were to: (1) verify the possible nonlinear effects on period ratios; (2) compare the general nonlinear characteristics of the theoretical light curves with the observed ones; (3) check the plausibility of the hypothesis o...

متن کامل

The galactic double–mode Cepheids I. Frequency analysis of the light curves and comparison with single–mode Cepheids

We submitted the available photometric V data of all the known galactic Double Mode Cepheids (DMCs) to a careful frequency analysis with the aim of detecting in each case the importance of the harmonics and of the cross coupling terms. For each object, starting from different data subsets, we progressively built a homogenous set of data, checking the consistency of the results step by step. It ...

متن کامل

The distance modulus of the Small Magellanic Cloud based on double-mode Cepheids

We employ the very recent photometric data of the ogle project together with stellar atmosphere and linear pulsation models to determine the distance modulus of the Small Magellanic Cloud from its double-mode Cepheids. Based on the requirement of obtaining the same distance modulus DM from the two types of variables (fundamental & first overtone and first & second overtone), we get DM = 19.05 m...

متن کامل

Magnitudes of Fundamental - Mode Cepheids from Single - Epoch Observations

We present an empirical method for converting single-point near-infrared J, H, and K measurements of fundamental-mode Cepheids to mean magnitudes, using complete light curves in V or I bands. The algorithm is based on the template light curves in the near-infrared bandpasses. The mean uncertainty of the method is estimated to about 0.03 mag, which is smaller than the uncertainties obtained in o...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

ژورنال

عنوان ژورنال: The Astronomical Journal

سال: 2022

ISSN: ['1538-3881', '0004-6256']

DOI: https://doi.org/10.3847/1538-3881/ac88d5