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jvillasr committed Oct 4, 2023
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2 changes: 1 addition & 1 deletion _config.yml
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Expand Up @@ -47,7 +47,7 @@ author-name: Jaime Villaseñor
# author-image: https://cdn.pixabay.com/photo/2015/10/05/22/37/blank-profile-picture-973460_960_720.png
author-image: https://raw.githubusercontent.com/jvillasr/jvillasr.github.io/master/assets/images/profilepic.png
# 60 Words About the Author
author-about: about the author - raw image (by JIV)
author-about:
# URL to the Author's Profile (i.e., Github, Twitter, Stackoverflow, etc)
author-url: https://github.com/jvillasr

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8 changes: 6 additions & 2 deletions _includes/about.html
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<img class="is-rounded" src="{{site.author-image}}" alt="{{site.author-name}}">
</figure>
</div>
<div class="column has-text-left-desktop has-text-left-tablet has-text-left-fullhd has-text-left-widescreen">
<p>{{site.author-about}}</p>
<div class="column has-text-left-desktop has-text-left-tablet has-text-left-fullhd has-text-left-widescreen has-space-btw-paragraphs">
<p>I'm deeply intrigued by the world of massive binary stars. My research focuses on exploring their multiplicity properties, orbital dynamics, and complex evolutionary pathways. To uncover the profound connection between these aspects, I rely mainly on spectroscopic surveys of massive stars.</p>

<p>Through meticulous analysis of the spectra of massive stars, I hunt for binary systems at various stages of their lives. Each discovery contributes to our understanding of how binarity shapes the lives of these remarkable massive entities.</p>

<p>Why massive binaries? Massive stars play a fundamental role in the Universe. Through their strong and hot winds, they completely alter their environment. Additionally, massive stars are the progenitors of exotic objects such as black holes and neutron stars. This means that in most cases, massive stars will explode as supernovae when forming those compact objects, enriching the interstellar medium and driving the chemical evolution of galaxies. Binarity adds even more excitement to the matter. By interacting with a close companion through mass exchange and mergers, the evolutionary paths of massive stars can drastically change, and this is the case for the majority of massive stars. Finally, in the last decade, a new dimension in the study of the cosmos has been confirmed: gravitational waves have been detected thanks to the Laser Interferometer Gravitational-Wave Observatory (LIGO) and the Virgo interferometer. Gravitational Waves are ripples in space-time that we can detect from very dense objects orbiting each other at very short distances. And guess what? These fascinating objects are exclusively produced by massive binary stars!</p>
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32 changes: 31 additions & 1 deletion _includes/resume.html
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Expand Up @@ -55,8 +55,38 @@ <h1 class="title has-text-primary">Education</h1>
<div class="thesis">"Evolution of Compact Binaries: The Future of Post-Common-Envelope Binaries"</div>
<div class="supervisor">Prof. Dr. Matthias Schreiber</div>
</div>
<h1 class="title has-text-primary">Publications</h1>
<h1 class="title has-text-primary">Selected Publications</h1>
<!-- Publications list goes here -->
<div class="resume-entry">
<h3 class="publ-title">The B-type Binaries Characterisation Programme - II. VFTS 291: a stripped star from a recent mass transfer phase</h3>
<p class="publ-authors"><span class="highlight">J. I. Villaseñor</span>, D. J. Lennon, A. Picco, T. Shenar, P. Marchant, N. Langer, P. L. Dufton, F. Nardini, C. J. Evans, J. Bodensteiner, S. E. de Mink, Y. Götberg, I. Soszyński, W. D. Taylor, and H. Sana</p>
<p class="publ-info"><a href="https://ui.adsabs.harvard.edu/abs/2023MNRAS.525.5121V/abstract" target="_blank">2023, MNRAS, 525, pp. 5121–5145</a></p>
</div>
<div class="resume-entry">
<h3 class="publ-title">Searching for compact objects in the single-lined spectroscopic binaries of the young Galactic cluster NGC 6231</h3>
<p class="publ-authors">G. Banyard, L. Mahy, H. Sana, J. Bodensteiner, <span class="highlight">J. I. Villaseñor</span>, K. Sen, N. Langer, S. de Mink, A. Picco, and T. Shenar</p>
<p class="publ-info"><a href="https://ui.adsabs.harvard.edu/abs/2023A%26A...674A..60B/abstract" target="_blank">2023, A&A, 674, A60</a></p>
</div>
<div class="resume-entry">
<h3 class="publ-title">The VLT-FLAMES survey of massive stars. NGC 2004#115: A triple system hosting a possible short period B+BH binary</h3>
<p class="publ-authors">D. J. Lennon, P. L. Dufton, <span class="highlight">J. I. Villaseñor</span>, C. J. Evans, N. Langer, R. Saxton, I. M. Monageng, and S. Toonen</p>
<p class="publ-info"><a href="https://ui.adsabs.harvard.edu/abs/2022A%26A...665A.180L/abstract" target="_blank">2022, A&A, 665, A180</a></p>
</div>
<div class="resume-entry">
<h3 class="publ-title">Properties of the Be-type stars in 30 Doradus</h3>
<p class="publ-authors">P. L. Dufton, D. J. Lennon, <span class="highlight">J. I. Villaseñor</span>, I. D. Howarth, C. J. Evans, S. E. de Mink, H. Sana, and W. D. Taylor</p>
<p class="publ-info"><a href="https://ui.adsabs.harvard.edu/abs/2022MNRAS.512.3331D/abstract" target="_blank">2022, MNRAS, 512, pp. 3331–3344</a></p>
</div>
<div class="resume-entry">
<h3 class="publ-title">The observed multiplicity properties of B-type stars in the Galactic young open cluster NGC 6231</h3>
<p class="publ-authors">G. Banyard, H. Sana, L. Mahy, J. Bodensteiner, <span class="highlight">J. I. Villaseñor</span>, and C. J. Evans</p>
<p class="publ-info"><a href="https://ui.adsabs.harvard.edu/abs/2022A%26A...658A..69B/abstract" target="_blank">2022, A&A, 658, A69</a></p>
</div>
<div class="resume-entry">
<h3 class="publ-title">The B-type binaries characterization programme I. Orbital solutions for the 30 Doradus population</h3>
<p class="publ-authors"><span class="highlight">J. I. Villaseñor</span>, W. D. Taylor, C. J. Evans, O. H. Ramı́rez-Agudelo, H. Sana, L. A. Almeida, S. E. de Mink, P. L. Dufton, and N. Langer</p>
<p class="publ-info"><a href="https://ui.adsabs.harvard.edu/abs/2021MNRAS.507.5348V/abstract" target="_blank">2021, MNRAS, 507, pp. 5348–5375</a></p>
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23 changes: 23 additions & 0 deletions assets/css/style.scss
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}

#about {
.has-space-btw-paragraphs {
/* Add space between paragraphs */
p {
margin-bottom: 15px; /* Adjust the value to control the spacing */
}
}
.image {
max-width: 20vmax;
margin: auto;
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color: rgb(213, 68, 249); /* Hover color for link */
}

.publ-title {
font-size: 18px;
}
.publ-authors {
font-size: 16px;
color: #989898;
margin-left: 30px
}
.highlight {
font-weight: bold;
color: #333;
}
.publ-info {
font-size: 14px;
font-style: italic;
margin-left: 30px
}
}


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