%0 Journal Article %1 WOS:000344550300069 %A Silva, J R P %A Soares, B B %A de Freitas, D B %C TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND %D 2014 %I IOP PUBLISHING LTD %J ASTROPHYSICAL JOURNAL %K fundamental parameters; rotation; stars: statistics} {stars: %N 1 %R 10.1088/0004-637X/796/1/69 %T CHANDRASEKHAR'S RELATION AND STELLAR ROTATION IN THE KEPLER FIELD %V 796 %X According to the statistical law of large numbers, the expected mean of identically distributed random variables of a sample tends toward the actual mean as the sample increases. Under this law, it is possible to test the Chandrasekhar's relation (CR), < V > = (pi/4)(-1) < Vsin i >, using a large amount of Vsin i and V data from different samples of similar stars. In this context, we conducted a statistical test to check the consistency of the CR in the Kepler field. In order to achieve this, we use three large samples of V obtained from Kepler rotation periods and a homogeneous control sample of Vsin i to overcome the scarcity of Vsin i data for stars in the Kepler field. We used the bootstrap-resampling method to estimate the mean rotations (< V > and < V sin i >) and their corresponding confidence intervals for the stars segregated by effective temperature. Then, we compared the estimated means to check the consistency of CR, and analyzed the influence of the uncertainties in radii measurements, and possible selection effects. We found that the CR with < sin i > = pi/4 is consistent with the behavior of the < V > as a function of Vsin i for stars from the Kepler field as there is a very good agreement between such a relation and the data.

@article{WOS:000344550300069, abstract = {According to the statistical law of large numbers, the expected mean of identically distributed random variables of a sample tends toward the actual mean as the sample increases. Under this law, it is possible to test the Chandrasekhar's relation (CR), < V > = (pi/4)(-1) < Vsin i >, using a large amount of Vsin i and V data from different samples of similar stars. In this context, we conducted a statistical test to check the consistency of the CR in the Kepler field. In order to achieve this, we use three large samples of V obtained from Kepler rotation periods and a homogeneous control sample of Vsin i to overcome the scarcity of Vsin i data for stars in the Kepler field. We used the bootstrap-resampling method to estimate the mean rotations (< V > and < V sin i >) and their corresponding confidence intervals for the stars segregated by effective temperature. Then, we compared the estimated means to check the consistency of CR, and analyzed the influence of the uncertainties in radii measurements, and possible selection effects. We found that the CR with < sin i > = pi/4 is consistent with the behavior of the < V > as a function of Vsin i for stars from the Kepler field as there is a very good agreement between such a relation and the data.}, added-at = {2022-05-23T20:00:14.000+0200}, address = {TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND}, author = {Silva, J R P and Soares, B B and de Freitas, D B}, biburl = {https://www.bibsonomy.org/bibtex/24667a075d34e21f78bdcb859464fd4b4/ppgfis_ufc_br}, doi = {10.1088/0004-637X/796/1/69}, interhash = {9f85fe9ae23a8419b5bc658a79bb7aef}, intrahash = {4667a075d34e21f78bdcb859464fd4b4}, issn = {0004-637X}, journal = {ASTROPHYSICAL JOURNAL}, keywords = {fundamental parameters; rotation; stars: statistics} {stars:}, number = 1, publisher = {IOP PUBLISHING LTD}, pubstate = {published}, timestamp = {2022-05-23T20:00:14.000+0200}, title = {CHANDRASEKHAR'S RELATION AND STELLAR ROTATION IN THE KEPLER FIELD}, tppubtype = {article}, volume = 796, year = 2014 }