* Absolute Magnitude: This measures a star's intrinsic brightness as seen from a standard distance of 10 parsecs (about 32.6 light-years).

* Magnitude Scale: The magnitude scale is logarithmic and *reversed*. Brighter objects have lower (more negative) magnitudes, while fainter objects have higher (more positive) magnitudes.

So, stars with large positive absolute magnitudes are intrinsically faint. They are often small, cool, red dwarf stars.

Here are some examples of stars with large positive absolute magnitudes:

* Proxima Centauri: Our closest stellar neighbor, a red dwarf with an absolute magnitude of +15.5.

* Barnard's Star: Another red dwarf, known for its high proper motion, with an absolute magnitude of +13.2.

* Wolf 359: Another red dwarf, famous for being a nearby flare star, with an absolute magnitude of +16.6.

Let me know if you have any other questions!