Here's the process:
1. Giant Molecular Cloud: The starting point is a huge cloud of gas and dust called a giant molecular cloud.
2. Protostar: Within the cloud, gravity pulls material together, forming a dense core. This core heats up, and the object becomes a protostar. This is where we start seeing the beginnings of a star, but it's not quite a star yet.
3. T Tauri Star: As the protostar continues to grow, it becomes a T Tauri star. This phase is characterized by strong winds and variability in brightness.
4. Main Sequence Star: Finally, the core of the T Tauri star becomes hot enough for nuclear fusion to start. At this point, it becomes a main sequence star, like our Sun.
So, rather than having a specific name before it's a star, it goes through various phases, each with its own characteristics.