update links

gvard · gvard · commit 6f78e4997887 · 2025-07-23T22:43:20.000+03:00
diff --git a/links/index.html b/links/index.html
@@ -409,43 +409,49 @@ <h2 id="neighbourhood">Ближайшее звездное окружение и
 <li><a href="https://youtu.be/ZdR37sMbvgw" target="_blank" rel="noopener noreferrer">Борис Штерн: о реальности межзвездных полетов</a>.
   <a href="https://youtu.be/o8FbMjH4pFM" target="_blank" rel="noopener noreferrer">Межзвездный перелет: на чем лететь</a>.
   <a href="https://youtu.be/wWD7YBgfuxo" target="_blank" rel="noopener noreferrer">Межзвездный перелет техника и сроки</a></li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2016ApJ...831...18C/abstract" target="_blank" rel="noopener noreferrer">Galactic Cosmic Rays in the Local Interstellar Medium: Voyager 1 Observations and Model Results</a> (2016),
-  <a href="https://ui.adsabs.harvard.edu/abs/2022SSRv..218...42R/abstract" target="_blank" rel="noopener noreferrer">Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium</a> (2022)</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2016ApJ...831...18C" target="_blank" rel="noopener noreferrer">Galactic Cosmic Rays in the Local Interstellar Medium: Voyager 1 Observations and Model Results</a> (2016),
+  <a href="https://ui.adsabs.harvard.edu/abs/2022SSRv..218...42R" target="_blank" rel="noopener noreferrer">Galactic Cosmic Rays Throughout the Heliosphere and in the Very Local Interstellar Medium</a> (2022)</li>
 <li><a href="https://arxiv.org/abs/1804.03698" target="_blank" rel="noopener noreferrer">Interstellar Escape from Proxima b is Barely Possible with Chemical Rockets</a>,
-  <a href="https://ui.adsabs.harvard.edu/abs/2018RNAAS...2..154L/abstract" target="_blank" rel="noopener noreferrer">Limitations of Chemical Propulsion for Interstellar Escape from Habitable Zones Around Low-mass Stars</a> (2018)</li>
+  <a href="https://ui.adsabs.harvard.edu/abs/2018RNAAS...2..154L" target="_blank" rel="noopener noreferrer">Limitations of Chemical Propulsion for Interstellar Escape from Habitable Zones Around Low-mass Stars</a> (2018)</li>
 <li>Ближайшие звезды:<br>
-  <a href="https://ui.adsabs.harvard.edu/abs/1940PA.....48..297V/abstract" target="_blank" rel="noopener noreferrer">List of Stars nearer than five parsecs</a> (1940)<br>
-  <a href="https://ui.adsabs.harvard.edu/abs/2018AJ....155..265H/abstract" target="_blank" rel="noopener noreferrer">The Solar Neighborhood XLIV: RECONS Discoveries within 10 Parsecs</a> (2018)</li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2012ApJ...753..156K/abstract" target="_blank" rel="noopener noreferrer">Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function</a> (2012). Окрестности 8 парсек:<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/1940PA.....48..297V" target="_blank" rel="noopener noreferrer">List of Stars nearer than five parsecs</a> (1940)<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/2018AJ....155..265H" target="_blank" rel="noopener noreferrer">The Solar Neighborhood XLIV: RECONS Discoveries within 10 Parsecs</a> (2018)</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2012ApJ...753..156K" target="_blank" rel="noopener noreferrer">Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function</a> (2012). Окрестности 8 парсек:<br>
   <img src="../stars/images/nearest8pc.png" width="500" title="The 8pc sample as a function of spectral type plotted in three ways – as total mass (left axis), mass density (right axis), and histogram (numbers above each star stack)" alt="The 8pc sample as a function of spectral type plotted in three ways – as total mass (left axis), mass density (right axis), and histogram (numbers above each star stack)"></li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2021A%26A...650A.201R/abstract" target="_blank" rel="noopener noreferrer">The 10 parsec sample in the Gaia era</a> (2021),
-  <a href="https://ui.adsabs.harvard.edu/abs/2022csss.confE.218R/abstract" target="_blank" rel="noopener noreferrer">The 10 parsec sample in the Gaia era: first update</a> (2023).
+<li><a href="https://ui.adsabs.harvard.edu/abs/2021A%26A...650A.201R" target="_blank" rel="noopener noreferrer">The 10 parsec sample in the Gaia era</a> (2021),
+  <a href="https://ui.adsabs.harvard.edu/abs/2022csss.confE.218R" target="_blank" rel="noopener noreferrer">The 10 parsec sample in the Gaia era: first update</a> (2023).
   <a href="https://nplus1.ru/news/2021/05/08/map-of-sun-neighbor" target="_blank" rel="noopener noreferrer">Окрестности 10 парсек</a>:<br>
   <img src="../stars/images/nearest10pc.png" width="500" alt="The 10pc sample" title="Распределение звезд и дозвездных объектов в окрестности 10 парсек по спектральным классам"></li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2021A%26A...649A...6G/abstract" target="_blank" rel="noopener noreferrer">Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars</a> (2021). Окрестности 100 пк.</li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2021ApJS..253....7K/abstract" target="_blank" rel="noopener noreferrer">The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs</a> (2021)</li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2023A%26A...670A..19G/abstract" target="_blank" rel="noopener noreferrer">The Fifth Catalogue of Nearby Stars</a> (CNS5, 2023). Окрестности 25 пк.</li>
-<li><a href="https://arxiv.org/abs/2312.03639" target="_blank" rel="noopener noreferrer">The Initial Mass Function Based on the Full-sky 20-pc Census of ~3,600 Stars and Brown Dwarfs</a> (2023). The 20-pc census enables us to identify the nearest star or brown dwarf in each constellation (Table B6).</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2021A%26A...649A...6G" target="_blank" rel="noopener noreferrer">Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars</a> (2021). Окрестности 100 пк.</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2021ApJS..253....7K" target="_blank" rel="noopener noreferrer">The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs</a> (2021)</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2023A%26A...670A..19G" target="_blank" rel="noopener noreferrer">The Fifth Catalogue of Nearby Stars</a> (CNS5, 2023). Окрестности 25 пк.</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2024ApJS..271...55K" target="_blank" rel="noopener noreferrer">The Initial Mass Function Based on the Full-sky 20 pc Census of ~3600 Stars and Brown Dwarfs</a> (2023-2024).
+  <a href="https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/271/55" target="_blank" rel="noopener noreferrer">Catalog</a>.
+  <ul>
+    <li>The 20 pc census enables us to identify the nearest star or brown dwarf in each constellation (Table B1)</li>
+    <li>The 20 pc census of objects colder than 600 K, corresponding to spectral type ~T8.5, is still incomplete beyond 15 pc, and the completeness volume shrinks to 11 pc at 450 K, corresponding to spectral type ~Y0 (Table 17)</li>
+    <li>Moreover, additional sources of incompleteness for objects as warm as 1350 K are high backgrounds and confusion along the Galactic plane (Section 7.1)</li>
+  </ul></li>
 </ul>
 
 <h3 id="neareststars">Ближе Проксимы: сближения звезд с Солнцем</h3>
 <ul>
-<li><a href="https://ui.adsabs.harvard.edu/abs/1994QJRAS..35....1M/abstract" target="_blank" rel="noopener noreferrer">The close approach of stars in the solar neighbourhood</a> (1994)</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/1994QJRAS..35....1M" target="_blank" rel="noopener noreferrer">The close approach of stars in the solar neighbourhood</a> (1994)</li>
 <li><a href="https://ru.wikipedia.org/wiki/%D0%97%D0%B2%D0%B5%D0%B7%D0%B4%D0%B0_%D0%A8%D0%BE%D0%BB%D1%8C%D1%86%D0%B0" target="_blank" rel="noopener noreferrer">Звезда Шольца</a>:
-  <a href="https://ui.adsabs.harvard.edu/abs/2015ApJ...800L..17M/abstract" target="_blank" rel="noopener noreferrer">The Closest Known Flyby of a Star to the Solar System</a> (2015)</li>
+  <a href="https://ui.adsabs.harvard.edu/abs/2015ApJ...800L..17M" target="_blank" rel="noopener noreferrer">The Closest Known Flyby of a Star to the Solar System</a> (2015)</li>
 <li><a href="https://ru.wikipedia.org/wiki/%D0%93%D0%BB%D0%B8%D0%B7%D0%B5_710" target="_blank" rel="noopener noreferrer">Глизе 710</a>,
   <a href="http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD%207977" target="_blank" rel="noopener noreferrer">HD 7977</a>:
-  <a href="https://ui.adsabs.harvard.edu/abs/2018A%26A...616A..37B/abstract" target="_blank" rel="noopener noreferrer">New stellar encounters discovered in the second Gaia data release</a> (2018),<br>
-  <a href="https://arxiv.org/abs/2207.06258" target="_blank" rel="noopener noreferrer">Stars that approach within one parsec of the Sun: New and more accurate encounters identified in Gaia Data Release 3</a> (2022)</li>
+  <a href="https://ui.adsabs.harvard.edu/abs/2018A%26A...616A..37B" target="_blank" rel="noopener noreferrer">New stellar encounters discovered in the second Gaia data release</a> (2018),<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/2022ApJ...935L...9B" target="_blank" rel="noopener noreferrer">Stars that approach within one parsec of the Sun: New and more accurate encounters identified in Gaia Data Release 3</a> (2022)</li>
 <li><a href="https://simbad.u-strasbg.fr/simbad/sim-id?Ident=WD+0810-353" target="_blank" rel="noopener noreferrer">WD 0810-353</a>:
-  <a href="https://ui.adsabs.harvard.edu/abs/2020AstL...46..245B/abstract" target="_blank" rel="noopener noreferrer">Analysis of Close Stellar Encounters with the Solar System</a> (2020),<br>
-  <a href="https://ui.adsabs.harvard.edu/abs/2021AstL...47..180B/abstract" target="_blank" rel="noopener noreferrer">Study of Close Stellar Encounters with the Solar System Based on Data from the Gaia EDR3 Catalogue</a> (2021),<br>
-  <a href="https://ui.adsabs.harvard.edu/abs/2022AstL...48..542B/abstract" target="_blank" rel="noopener noreferrer">Search for close encounters of stars with the Solar System using Gaia DR3 catalog</a> (2022)<br>
-  <a href="https://ui.adsabs.harvard.edu/abs/2023ApJ...952..129L/abstract" target="_blank" rel="noopener noreferrer">Not So Fast, Not So Furious: Just Magnetic</a>.
+  <a href="https://ui.adsabs.harvard.edu/abs/2020AstL...46..245B" target="_blank" rel="noopener noreferrer">Analysis of Close Stellar Encounters with the Solar System</a> (2020),<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/2021AstL...47..180B" target="_blank" rel="noopener noreferrer">Study of Close Stellar Encounters with the Solar System Based on Data from the Gaia EDR3 Catalogue</a> (2021),<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/2022AstL...48..542B" target="_blank" rel="noopener noreferrer">Search for close encounters of stars with the Solar System using Gaia DR3 catalog</a> (2022)<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/2023ApJ...952..129L" target="_blank" rel="noopener noreferrer">Not So Fast, Not So Furious: Just Magnetic</a>.
   There will probably be no close encounter between the solar system and WD 0810-353. We also reject the suggestion that the star is a hypervelocity runaway star, a survivor of a Type Ia supernova explosion. It is just a stellar remnant in the solar neighborhood with a very strong and complex magnetic field.
   Also, <a href="https://www.eso.org/public/blog/rogue-star/" target="_blank" rel="noopener noreferrer">Rogue star not heading for Solar System collision after all</a></li>
-<li><a href="https://arxiv.org/abs/2109.07549" target="_blank" rel="noopener noreferrer">Galactic and stellar perturbations of long period comet motion - Practical considerations</a> (2021)<br>
-  <a href="https://arxiv.org/abs/2206.11047" target="_blank" rel="noopener noreferrer">Important stellar perturbers found during the StePPeD database update based on Gaia EDR3 data</a> (2022)</li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2022A%26A...657A..65D" target="_blank" rel="noopener noreferrer">Galactic and stellar perturbations of long period comet motion - Practical considerations</a> (2021)<br>
+  <a href="https://ui.adsabs.harvard.edu/abs/2022A%26A...664A.123D" target="_blank" rel="noopener noreferrer">Important stellar perturbers found during the StePPeD database update based on Gaia EDR3 data</a> (2022)</li>
 </ul>
 
 <h2 id="interstellar">Проблемы межзвездных перелетов</h2>
@@ -503,7 +509,7 @@ <h3 id="food">Космическая еда</h3>
   <a href="https://cipotato.org/" target="_blank" rel="noopener noreferrer">International Potato Center</a></li>
 <li><a href="https://www.algomed.de/ru/%D1%85%D0%BB%D0%BE%D1%80%D0%B5%D0%BB%D0%BB%D0%B0/" target="_blank" rel="noopener noreferrer">Хлорелла</a>: разрушение клеточных оболочек хлореллы не изменяет ее исходные характеристики и физиологические эффекты.</li>
 <li><a href="https://pubmed.ncbi.nlm.nih.gov/21554801/" target="_blank" rel="noopener noreferrer">Insect food for astronauts: gas exchange in silkworms fed on mulberry and lettuce and the nutritional value of these insects for human consumption during deep space flights</a></li>
-<li><a href="https://ui.adsabs.harvard.edu/abs/2016cosp...41E.952K/abstract" target="_blank" rel="noopener noreferrer">Usefulness of the insect food in the long-term space stay</a></li>
+<li><a href="https://ui.adsabs.harvard.edu/abs/2016cosp...41E.952K" target="_blank" rel="noopener noreferrer">Usefulness of the insect food in the long-term space stay</a></li>
 <li><a href="https://www.nature.com/articles/s43016-022-00530-x" target="_blank" rel="noopener noreferrer">A hybrid inorganic–biological artificial photosynthesis system for energy-efficient food production</a> (2022)</li>
 </ul>
 
