... BMI BMI ≤ −2 SD at 24 months or current use of a feeding tube or cyproheptadine for appetite stimulation Notes: SD = standard deviation. Adapted from “Diagnosis and management of Silver–Russell syndrome: first international consensus statement,” by E.L. Wakeling, F...

... late type stars. stars: emission-line, Be stars: circumstellar matter stars: fundamental parameters Hertzprung-Russell and colour-magnitude diagrams A Photometric Comparison of B and Be stars using Gaia DR3 Isaac C. Radley1 , René D. Oudmaijer2,1, Miguel Vioque3, and Jonathan M. Dodd1 1School...

... is mainly populated by fast-rotating stars. galaxies: star clusters: general Magellanic Clouds stars: rotation stars: evolution Hertzsprung Russell and colour magnitude diagrams open clusters and associations: general O RIG IN AL UN ED ITED M A N USCRIPT Strikingly high fraction of fast rotators...

... its member stars, including high-mass stars. However, no clear tidal tails can be detected around the cluster. Hertzsprung–Russell and C–M diagrams methods: statistical open clusters and associations: individual (NGC 2506) parallaxes proper motions Foundation of Changzhou University YPC24020219...

... the difference for objects younger than . Hertzsprung–Russell and colour–magnitude diagrams stars: horizontal branch open clusters and associations: general galaxies: stellar content FAPEMIG 10.13039/501100004901 CNPq 10.13039/501100003593 440142/2022-9 404482/2021-0 CAPES 10.13039...

... be driven by contamination due to the  pc span of the cylinder in distance. supernovae Hertzsprung–Russell and colour–magnitude diagrams supernovae: general supernovae: individual ISM: supernova remnants NASA 10.13039/100000104 80NSSC23K1444 European Space Agency 10.13039/501100000844...

.... These findings are consistent with a scenario where 2P stars form in a more centrally concentrated environment, where the interaction with the Milky Way tidal field plays a crucial role in the dynamical evolution of MPs, especially of 1P. Hertzsprung–Russell and colour–magnitude diagrams stars: kinematics...

...Eloïse Giabicani; Amélie Perriere; Irène Netchine The authors have no conflicts of interest and no disclosures. References 1 Vimercati   A , Tannorella   P , Guzzetti   S , et al   Distinguishing genetic alterations versus (epi)mutations in Silver-Russell syndrome and focus...

..., . methods: data analysis methods: statistical binaries: general Hertzsprung–Russell and colour–magnitude diagrams open clusters and associations: general Binary star systems have an enhanced effect on the evolution of star clusters when compared to single star systems. For instance, Hurley et al...

...A H Sheikh; Simanta Deka; Biman J Medhi methods: statistical stars: formation stars: fundamental parameters Hertzsprung–Russell and colour–magnitude stars: pre-main-sequence dust, extinction This region offers a rich environment for studying triggered star formation, driven by the interaction...

... protoplanetary discs Hertzsprung–Russell and colour–magnitude diagrams stars: low-mass stars: pre-main-sequence techniques: photometric NASA 10.13039/100000104 National Science Foundation 10.13039/100000001 MINECO 10.13039/501100003329 AyA2017-84089 776403 DST 10.13039/501100008789...

.../ ), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. See the journal About page for additional terms. Abstract Context Silver–Russell Syndrome (SRS) is a growth retardation disorder characterized by pre- and postnatal growth...

... Hertzsprung–Russell and colour–magnitude diagrams ultraviolet: stars NASA 10.13039/100000104 European Space Agency 10.13039/501100000844 DPAC 10.13039/100018121 DST 10.13039/501100001409 IF230175 Old open clusters are ideal laboratories for studying stellar populations...

... relaxation. We estimate that the observed tidal tails could have formed within the last 30 Myr. Hertzsprung–Russell and C-M diagrams methods: statistical open clusters and associations: individual (NGC 2112) parallaxes proper motions Foundation of Changzhou University KYCX24_3233 KYP2202231C...

... of these clusters, highlighting the consistency between the derived metallicity and spectroscopic determinations from various sources. methods: statistical Hertzsprung–Russell and colour–magnitude diagrams galaxies: star clusters: general CNPq 10.13039/501100003593 140642/2021-8 141875/2023-2 404482/2021-0...

... in a cluster age of Gyr. Hertzsprung–Russell and colour–magnitude diagrams open clusters and associations: individual: M67 In this paper, we aim to develop a new theoretical isochrone that incorporates the latest research on the physics governing stellar evolution: notably, model improvements based...

... caution in determining the ages of young clusters from non-rotating isochrones, as neglecting the effects of stellar rotation can impact the isochrone dating by up to factors of 5–20 per cent. Stars: evolution Hertzsprung–Russell and colour–magnitude diagrams Stars: rotation open clusters...

... ) possibly due to the magnetic braking of their rotations. techniques: spectroscopic Hertzsprung–Russell and colour–magnitude diagrams stars: rotation open clusters and associations: individual: NGC 2355 Chinese Academy of Sciences 10.13039/501100002367 CAS 10.13039/100005542 Natural...

... the efficiency score’. They introduced a general inverse non-radial DEA model where slacks play an important role. Jahanshahloo et al. (2014) studied the inverse DEA using the non-radial Enhanced Russell Model (ERM) and introduced a new problem: ‘among a group of DMUs, how much should the input...

... permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. See the journal About page for additional terms. Abstract Silver-Russell syndrome (SRS) is a clinical diagnosis requiring the fulfillment of ≥ 4/6 Netchine-Harbison Clinical Scoring...