Spartan Daily, October 29, 1940

Volume 29, Issue 29https://scholarworks.sjsu.edu/spartandaily/3191/thumbnail.jp

Spartan Daily, October 29, 1940

Volume 29, Issue 29https://scholarworks.sjsu.edu/spartandaily/3191/thumbnail.jp

Making Aid Effectiveness Work for Family Planning and Reproductive Health

This Population Action International Working Paper analyzes the five principles of aid effectiveness -- country ownership, alignment, harmonization, managing for results, and mutual accountability -- from a family planning and reproductive health perspective. It also describes how the Paris Declaration has changed the ways of managing and delivering aid; highlights entry points and obstacles for champions working to improve funding and policies; and makes recommendations for civil society organizations, governments and donors

A note on "new travelling wave solutions to the Ostrovsky equation"

In a recent paper by Yaşar [E. Yaşar, New travelling wave solutions to the Ostrovsky equation, Appl. Math. Comput. 216 (2010), 3191-3194], 'new' travelling-wave solutions to the transformed reduced Ostrovsky equation are presented. In this note it is shown that some of these solutions are disguised versions of known solutions

The host of the Type I SLSN 2017egm: A young, sub-solar metallicity environment in a massive spiral galaxy

Here we present an integral-field study of the massive, high-metallicity spiral NGC 3191, the host of SN 2017egm, the closest SLSN Type I to date. We use data from PMAS/CAHA and the public MaNGA survey to shed light on the properties of the SLSN site and the origin of star-formation in this non-starburst spiral galaxy. We map the physical properties different \ion{H}{II} regions throughout the galaxy and characterize their stellar populations using the STARLIGHT fitting code. Kinematical information allows to study a possible interaction with its neighbouring galaxy as the origin of recent star formation activity which could have caused the SLSN. NGC 3191 shows intense star-formation in the western part with three large SF regions of low metallicity. The central regions of the host have a higher metallicity, lower specific star-formation rate and lower ionization. Modeling the stellar populations gives a different picture: The SLSN region has two dominant stellar populations with different ages, the youngest one with an age of 2-10 Myr and lower metallicity, likely the population from which the SN progenitor originated. Emission line kinematics of NGC 3191 show indications of interaction with its neighbour MCG+08-19-017 at $\sim$45 kpc, which might be responsible for the recent starburst. In fact, this galaxy pair has in total hosted 4 SNe, 1988B (Type Ia), SN 2003ds (Type Ic in MCG+08-19-017), PTF10bgl (SLSN-Type II) and 2017egm, underlying the enhanced SF in both galaxies due to interaction. Our study shows that one has to be careful interpreting global host and even gas properties without looking at the stellar population history of the region. SLSNe seem to still be consistent with massive stars ($>$ 20 M$_\odot$) requiring low ($< 0.6Z_{\odot}$) metallicity and those environments can also occur in massive, late-type galaxies but not necessarily starbursts.Comment: Accepted for publication in A&A, 13 pages, 11 figures, 7 tables. Abstract has been reduced to match arXiv form requirement

Xavier University Newswire

https://www.exhibit.xavier.edu/student_newspaper/3191/thumbnail.jp

Las Vegas Optic, 01-05-1914

https://digitalrepository.unm.edu/lvdo_news/3191/thumbnail.jp

If You Can\u27t Get A Girl A Girl In The Summertime : You\u27ll Never Get A All

https://digitalcommons.library.umaine.edu/mmb-vp/3191/thumbnail.jp

State v. Mantz Appellant\u27s Brief Dckt. 35540

https://digitalcommons.law.uidaho.edu/idaho_supreme_court_record_briefs/3191/thumbnail.jp

MGRRE_ThinSections_MGRRE-6_007

https://scholarworks.wmich.edu/tsi/3191/thumbnail.jp